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712.3179 | Mario I. Molina | Mario I. Molina, Yaroslav V. Kartashov, Lluis Torner, and Yuri S.
Kivshar | Surface solitons in two-dimensional chirped photonic lattices | 12 pages, 7 figures | Phys. Rev. A 77, 053813 (2008) | 10.1364/OL.32.002668 | null | nlin.PS | null | We study surface modes in semi-infinite chirped two-dimensional photonic
lattices in the frame- work of an effective discrete nonlinear model. We
demonstrate that the lattice chirp can change dramatically the conditions for
the mode localization near the surface, and we find numerically the families of
surface modes, in linear lattices, and discrete surface solitons, in nonlinear
lattices. We demonstrate that, in a sharp contrast to one-dimensional discrete
surface solitons, in two-dimensional lattices the mode threshold power is
lowered by the action of both the surface and lattice chirp. By manipulating
with the lattice chirp, we can control the mode position and its localization.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:03:47 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Molina",
"Mario I.",
""
],
[
"Kartashov",
"Yaroslav V.",
""
],
[
"Torner",
"Lluis",
""
],
[
"Kivshar",
"Yuri S.",
""
]
] | [
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712.318 | Halton Arp | H. Arp | Dark Energy and the Hubble Constant | 3 Figures, 7 pages | null | null | null | astro-ph | null | Dark energy is inferred from a Hubble expansion which is slower at epochs
which are earlier than ours. But evidence reviewed here shows $H_0$ for nearby
galaxies is actually less than currently adopted and would instead require {\it
deceleration} to reach the current value.
Distances of Cepheid variables in galaxies in the Local Supercluster have
been measured by the Hubble Space Telescope and it is argued here that they
require a low value of $H_0$ along with redshifts which are at least partly
intrinsic. The intrinsic component is hypothesized to be a result of the
particle masses increasing with time.
The same considerations apply to Dark Matter. But with particle masses
growing with time, the condensation from plasmoid to proto galaxy not only does
away with the need for unseen ``dark matter'' but also explains the intrinsic
(non-velocity) redshifts of younger matter.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:10:02 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Arp",
"H.",
""
]
] | [
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712.3181 | Hung The Diep | X. T. Pham Phu (LPTM), V. Thanh Ngo (IOP, Apctp), H. T. Diep (LPTM) | Critical behavior of magnetic thin films as a function of thickness | 10 pages, 19 figures | null | null | null | cond-mat.mtrl-sci | null | We study the critical behavior of magnetic thin films as a function of the
film thickness. We use the ferromagnetic Ising model with the high-resolution
multiple histogram Monte Carlo (MC) simulation. We show that though the 2D
behavior remains dominant at small thicknesses, there is a systematic
continuous deviation of the critical exponents from their 2D values. We observe
that in the same range of varying thickness the deviation of the exponent $\nu$
is rather small, while exponent $\beta$ suffers a larger deviation. We explain
these deviations using the concept of "effective" exponents suggested by
Capehart and Fisher in a finite-size analysis. The shift of the critical
temperature with the film thickness obtained here by MC simulation is in an
excellent agreement with their prediction.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:11:22 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Phu",
"X. T. Pham",
"",
"LPTM"
],
[
"Ngo",
"V. Thanh",
"",
"IOP, Apctp"
],
[
"Diep",
"H. T.",
"",
"LPTM"
]
] | [
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] |
712.3182 | Ping Dong | Ping Dong, Ming Yang, and Zhuo-Liang Cao | Quantum computation with quantum-dot spin qubits inside a cavity | Four pages and 1 figure | null | null | null | quant-ph | null | Universal set of quantum gates are realized from the conduction-band electron
spin qubits of quantum dots embedded in a microcavity via two-channel Raman
interaction. All of the gate operations are independent of the cavity mode
states, \emph{i.e.}, insensitive to the thermal cavity field. Individual
addressing and effective switch of the cavity mediated interaction are directly
possible here. Meanwhile, gate operations also can be carried out in parallel.
The simple realization of needed interaction for selective qubits makes current
scenario more suitable for scalable quantum computation.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:11:54 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Dong",
"Ping",
""
],
[
"Yang",
"Ming",
""
],
[
"Cao",
"Zhuo-Liang",
""
]
] | [
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] |
712.3183 | Bruce Yabsley | B.D. Yabsley | Double ccbar production in e+e- annihilations at high energy | 5 pages, 5 figures. To be published in the proceedings of CHARM07,
Ithaca, NY, August 2007, eConf C070805 | ECONF C070805:03,2007 | null | null | hep-ex hep-ph | null | We review the current state of experimental knowledge on double ccbar
production in e+e- annihilation. The large cross-sections (O(20 fb)) for e+e-
-> gamma* -> psi(') ccbar_{res} processes have been confirmed by detailed tests
and reproduced by a second group: they should now be considered
well-established. The latest experimental results concern the case where the
second ccbar system is above open-charm threshold: hidden-charm states continue
to play a prominent role in the mass spectrum. Some ``loose ends'' in the field
are also briefly discussed.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:15:43 GMT"
}
] | 2011-06-15T00:00:00 | [
[
"Yabsley",
"B. D.",
""
]
] | [
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] |
712.3184 | Horia Cornean | Philippe Briet, Horia D. Cornean, Delphine Louis | Diamagnetic expansions for perfect quantum gases II: uniform bounds | To appear in Asymptotic Analysis | null | null | null | math-ph cond-mat.mtrl-sci math.MP | null | Consider a charged, perfect quantum gas, in the effective mass approximation,
and in the grand-canonical ensemble. We prove in this paper that the
generalized magnetic susceptibilities admit the thermodynamic limit for all
admissible fugacities, uniformly on compacts included in the analyticity domain
of the grand-canonical pressure.
The problem and the proof strategy were outlined in \cite{3}. In \cite{4} we
proved in detail the pointwise thermodynamic limit near $z=0$. The present
paper is the last one of this series, and contains the proof of the uniform
bounds on compacts needed in order to apply Vitali's Convergence Theorem.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:20:31 GMT"
}
] | 2010-06-23T00:00:00 | [
[
"Briet",
"Philippe",
""
],
[
"Cornean",
"Horia D.",
""
],
[
"Louis",
"Delphine",
""
]
] | [
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712.3185 | Thierry Jolicoeur | Brice Chung, Thierry Jolicoeur | Fermions out of Dipolar Bosons in the lowest Landau level | 12 pages, 5 figures, published version | Phys. Rev. A77, 043608 (2008) | 10.1103/PhysRevA.77.043608 | null | cond-mat.mes-hall | null | In the limit of very fast rotation atomic Bose-Einstein condensates may
reside entirely in the lowest two-dimensional Landau level (LLL). For small
enough filling factor of the LLL, one may have formation of fractional quantum
Hall states. We investigate the case of bosons with dipolar interactions as may
be realized with Chromium-52 atoms. We show that at filling factor equal to
unity the ground state is a Moore-Read (a.k.a Pfaffian) paired state as is the
case of bosons with purely s-wave scattering interactions. This Pfaffian state
is destabilized when the interaction in the s-wave channel is small enough and
the ground state is a stripe phase with unidimensional density modulation. For
filling factor 1/3, we show that there is formation of a Fermi sea of
``composite fermions''. These composites are made of one boson bound with three
vortices. This phase has a wide range of stability and the effective mass of
the fermions depends essentially only of the scattering amplitude in momentum
channels larger or equal to 2. The formation of such a Fermi sea opens up a new
possible route to detection of the quantum Hall correlations.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:27:57 GMT"
},
{
"version": "v2",
"created": "Tue, 15 Apr 2008 08:29:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chung",
"Brice",
""
],
[
"Jolicoeur",
"Thierry",
""
]
] | [
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712.3186 | Mihnea Popa | Lawrence Ein and Mihnea Popa | Global division of cohomology classes via injectivity | 10 pages; dedication included, and minor corrections made; to appear
in the Michigan Math. J. volume in honor of Mel Hochster's 65th birthday | null | null | null | math.AG math.CV | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We note that the vanishing and injectivity theorems of Koll\'ar and
Esnault-Viehweg can be used to give a quick algebraic proof of a strengthening
of the Ein-Lazarsfeld Skoda-type division theorem for global sections of
adjoint line bundles vanishing along suitable multiplier ideal sheaves, and to
extend it to higher cohomology classes as well. For global sections, this is
also a slightly more general statement of the algebraic translation of an
analytic result of Siu. Along the way we write down an injectivity statement
for multiplier ideals, and its standard consequences.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:21:53 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Aug 2008 18:10:33 GMT"
}
] | 2008-08-18T00:00:00 | [
[
"Ein",
"Lawrence",
""
],
[
"Popa",
"Mihnea",
""
]
] | [
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712.3187 | Florent Chazel | Florent Chazel | On the Korteweg-de Vries approximation for uneven bottoms | null | European Journal of Mechanics / B Fluids 28 (2009), pp. 234-252 | 10.1016/j.euromechflu.2008.10.003 | null | math.AP physics.ao-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we focus on the water waves problem for uneven bottoms on a
two-dimensionnal domain. Starting from the symmetric Boussinesq systems derived
in [Chazel, Influence of topography on long water waves, 2007], we recover the
uncoupled Korteweg-de Vries (KdV) approximation justified by Schneider and
Wayne for flat bottoms, and by Iguchi in the context of bottoms tending to zero
at infinity at a substantial rate. The goal of this paper is to investigate the
validity of this approximation for more general bathymetries. We exhibit two
kinds of topography for which this approximation diverges from the Boussinesq
solutions. A topographically modified KdV approximation is then proposed to
deal with such bathymetries. Finally, all the models involved are numerically
computed and compared.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:51:17 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Dec 2007 15:01:37 GMT"
},
{
"version": "v3",
"created": "Thu, 3 Jan 2008 13:52:18 GMT"
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{
"version": "v4",
"created": "Fri, 5 Dec 2008 14:59:54 GMT"
},
{
"version": "v5",
"created": "Mon, 2 Feb 2009 13:04:56 GMT"
}
] | 2009-02-02T00:00:00 | [
[
"Chazel",
"Florent",
""
]
] | [
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] |
712.3188 | Alexander E. Shalyt-Margolin | A. E. Shalyt-Margolin | Vacuum Energy Problem, Fundamental Length and Deformed Quantum Field
Theory | 12 pages | null | null | null | gr-qc | null | The cosmological constant (vacuum energy) problem is analyzed within the
scope of quantum theories with UV-cut-off or fundamental length. Various cases
associated with the appearance of the latter are considered both using the
Generalized Uncertainty Relations and the deformed density matrix,previously
introduced in the author's works. The use of the deformed density matrix is
examined in detail. It is demonstrated that, provided the Fischler-Susskind
cosmic holographic conjecture is valid, the Vacuum Energy Density takes a value
close to the experimental one. The arguments supporting the validity of this
conjecture are given on the basis of the recently obtained results on
Gravitational Holography.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:53:03 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Shalyt-Margolin",
"A. E.",
""
]
] | [
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] |
712.3189 | S. B. Rutkevich | S. B. Rutkevich | Energy spectrum of bound-spinons in the quantum Ising spin-chain
ferromagnet | 33 pages, 8 figures | J. Stat. Phys., Vol. 131, N5, 917-939 (2008) | 10.1007/s10955-008-9495-1 | null | cond-mat.stat-mech | null | We study the excitation energy spectrum in the S=1/2 ferromagnetic Ising spin
chain with the easy axis z in a magnetic field h={h_x,0,h_z}. According to Wu
and McCoy's scenario of weak confinement, the fermionic spinon excitations
(kinks), being free at h_z = 0 in the ordered phase, are coupled into bosonic
bound states at arbitrary small h_z. We calculate the energy spectrum of such
excitations in the leading order in small h_z, using different perturbative
methods developed for the similar problem in the Ising field theory.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:24:05 GMT"
}
] | 2008-05-05T00:00:00 | [
[
"Rutkevich",
"S. B.",
""
]
] | [
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] |
712.319 | Helmut Dannerbauer | H. Dannerbauer, F. Walter, G. Morrison | Interferometric detections of GOODS 850-5 at 1 mm and 1.4 GHz | Accepted for publication by ApJL (12 pages, 1 figure). The resolution
of figure 1 has been degraded. A higher quality pdf version of this paper is
available at http://www.mpia-hd.mpg.de/homes/dannerb/ | null | 10.1086/528794 | null | astro-ph | null | We have obtained a position (at sub-arcsecond accuracy) of the submillimeter
bright source GOODS 850-5 (also known as GN10) in the GOODS North field using
the IRAM Plateau de Bure interferometer at 1.25 mm wavelengths (MM
J123633+6214.1, flux density: S(1.25 mm)=5.0+-1.0 mJy). This source has no
optical counterpart in deep ACS imaging down to a limiting magnitude of
i(775)=28.4 mag and its position is coincident with the position found in
recent sub-millimeter mapping obtained at the SMA (Wang et al. 2007). Using
deep VLA imaging at 20 cm, we find a radio source (S(20 cm)=32.7+-4.3 microJy)
at the same position that is significantly brighter than reported in Wang et
al. The source is detected by Spitzer in IRAC as well as at 24 microns. We
apply different photometric redshift estimators using measurements of the
dusty, mid/far-infrared part of the SED and derive a redshift z~4. Given our
detection in the millimeter and radio we consider a significantly higher
redshift (e.g., z~6 Wang et al. 2007) unlikely. MM J123633+6214.1 alias GOODS
850-5 nevertheless constitutes a bright representative of the high-redshift
tail of the submillimeter galaxy population that may contribute a significant
fraction to the (sub)millimeter background.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:07:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dannerbauer",
"H.",
""
],
[
"Walter",
"F.",
""
],
[
"Morrison",
"G.",
""
]
] | [
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712.3191 | Lucia Cavallasca | Roberto Artuso, Lucia Cavallasca, Giampaolo Cristadoro | Intermittency in two dimensions | 9 pages, 11 figures | null | null | null | nlin.CD | null | We introduce a family of area-preserving maps representing a (non-trivial)
two-dimensional extension of the Pomeau-Manneville family in one dimension. We
analyze the long-time behavior of recurrence time distributions and
correlations, providing analytical and numerical estimates. We study the
transport properties of a suitable lift and use a probabilistic argument to
derive the full spectrum of transport moments. Finally the dynamical effects of
a stochastic perturbation are considered.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 13:59:46 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Artuso",
"Roberto",
""
],
[
"Cavallasca",
"Lucia",
""
],
[
"Cristadoro",
"Giampaolo",
""
]
] | [
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] |
712.3192 | Mihnea Popa | Mihnea Popa | Generalized theta linear series on moduli spaces of vector bundles on
curves | 33 pages; made a few minor corrections and improvements, and added
some new results in the last section; written for the Handbook of Moduli | null | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This article is based on lecture notes prepared for the August 2006 Cologne
Summer School. The first part contains background material and references for
beginners. The second (and main) part is a survey of the current status in the
theory of pluri-theta linear series and generalized theta divisors on moduli
spaces of vector bundles on curves. It emphasizes relatively new techniques
employed in the analysis of linear series on these moduli spaces, namely the
use of moduli spaces of stable maps for understanding Quot schemes, and the
Fourier-Mukai functor in the study of coherent sheaves on abelian varieties. In
addition, it briefly describes recent important developments, most significant
of which is the proof of the Strange Duality conjecture due to Belkale and
Marian-Oprea.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:00:11 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Jan 2008 18:03:21 GMT"
},
{
"version": "v3",
"created": "Thu, 7 Feb 2008 16:31:09 GMT"
},
{
"version": "v4",
"created": "Sun, 17 Jan 2010 23:31:46 GMT"
}
] | 2010-01-18T00:00:00 | [
[
"Popa",
"Mihnea",
""
]
] | [
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712.3193 | Ivanov Dmitry | D.Yu. Ivanov | Exclusive vector meson electroproduction | 7 pages; Talk given at 12th International Conference on Elastic and
Diffractive Scattering: Forward Physics and QCD, Hamburg, DESY, Germany,
21-25 May 2007 | null | null | null | hep-ph | null | We discuss exclusive vector meson electroproduction within the QCD collinear
factorization framework. In Bjorken kinematics the amplitude factorizes in a
convolution of the nonperturbative meson distribution amplitude and the
generalized parton densities with the perturbatively calculable hard-scattering
amplitudes, which are presently known to next-to-leading order (NLO). At small
$x_{\rm B}$ NLO corrections are very large. It is related to appearance of BFKL
type logarithms in the hard-scattering amplitudes, that calls for a resummation
of these effects at higher orders. Here we report the first results of such
resummation.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:29:32 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Ivanov",
"D. Yu.",
""
]
] | [
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] |
712.3194 | Harold Steinacker | Harold Steinacker | Emergent 4D Gravity from Matrix Models | 5 pages. Based on talks given at the BW2007 workshop "Challenges
Beyond the Standard Model", Kladovo, Serbia and the Vienna Central European
Seminar "Particle Physics and quantum field theory" 2007 and the workshop
"Field Theory, Non-commutative Geometry and Strings", Zagreb, Croatia:
November 9-11, 2007 | Fortsch.Phys.56:510-515,2008 | 10.1002/prop.200710527 | null | hep-th | null | Recent progress in the understanding of gravity on noncommutative spaces is
discussed. A gravity theory naturally emerges from matrix models of
noncommutative gauge theory. The effective metric depends on the dynamical
Poisson structure, absorbing the degrees of freedom of the would-be U(1) gauge
field. The gravity action is induced upon quantization.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:10:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Steinacker",
"Harold",
""
]
] | [
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712.3195 | Pierre Jop | Pierre Jop (LPMCN, Iusti) | Hydrodynamic modeling of granular flows in a modified Couette cell | 4 pages | null | 10.1103/PhysRevE.77.032301 | null | cond-mat.soft | null | We present simulations of granular flows in a modified Couette cell, using a
continuum model recently proposed for dense granular flows. Based on a friction
coefficient, which depends on an inertial number, the model captures the
positions of the wide shear bands. We show that a smooth transition in
velocity-profile shape occurs when increasing the height of the granular
material, leading to a differential rotation of the central part close to the
surface. The numerical predictions are in qualitative agreement with previous
experimental results. The model provides predictions for the increase of the
shear bands width when increasing the rotation rate.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:12:09 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Jop",
"Pierre",
"",
"LPMCN, Iusti"
]
] | [
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] |
712.3196 | Daniel Garcia-Sanchez | D. Garcia-Sanchez, A. San Paulo, M.J. Esplandiu, F. Perez-Murano, L.
Forro, A. Aguasca, A. Bachtold | Mechanical detection of carbon nanotube resonator vibrations | null | Published in Phys. Rev. Lett. 99, 085501 (2007) | 10.1103/PhysRevLett.99.085501 | null | cond-mat.mes-hall | null | Bending-mode vibrations of carbon nanotube resonator devices were
mechanically detected in air at atmospheric pressure by means of a novel
scanning force microscopy method. The fundamental and higher order bending
eigenmodes were imaged at up to 3.1GHz with sub-nanometer resolution in
vibration amplitude. The resonance frequency and the eigenmode shape of
multi-wall nanotubes are consistent with the elastic beam theory for a doubly
clamped beam. For single-wall nanotubes, however, resonance frequencies are
significantly shifted, which is attributed to fabrication generating, for
example, slack. The effect of slack is studied by pulling down the tube with
the tip, which drastically reduces the resonance frequency.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:13:22 GMT"
}
] | 2012-07-12T00:00:00 | [
[
"Garcia-Sanchez",
"D.",
""
],
[
"Paulo",
"A. San",
""
],
[
"Esplandiu",
"M. J.",
""
],
[
"Perez-Murano",
"F.",
""
],
[
"Forro",
"L.",
""
],
[
"Aguasca",
"A.",
""
],
[
"Bachtold",
"A.",
""
]
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] |
712.3197 | Li Yang | Li Yang and Yufu Chen | An Upper Bound to the Number of Gates on Single Qubit within One
Error-Correction Period of Quantum Computation | null | null | null | null | quant-ph | null | Based on the amplitude behavior of quantum Rabi oscillation driven by a
coherent field we show that there exists an upper bound to the number of
logical operation performed on any single qubit within one error-correction
period of a quantum computation. We introduce a parameter to depict the maximum
of this number and estimate its decoherence limit. The analysis shows that a
generally accepted error-rate threshold of quantum logic gates limits the
parameter to so small a number that even a double of fault-tolerant Toffoli
gates can hardly be implemented reliably within one error-correction period.
This result suggests that the design of feasible fault-tolerant quantum
circuits is still an arduous task.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:20:12 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Dec 2007 10:10:53 GMT"
}
] | 2007-12-26T00:00:00 | [
[
"Yang",
"Li",
""
],
[
"Chen",
"Yufu",
""
]
] | [
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] |
712.3198 | Ivan Struchiner | Rui Loja Fernandes and Ivan Struchiner | Lie Algebroids and Classification Problems in Geometry | 16 pages; research announcement; final version to appear in Sao Paulo
Journal of Mathematical Sciences | null | null | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We show how one can associate to a given class of finite type G-structures a
classifying Lie algebroid. The corresponding Lie groupoid gives models for the
different geometries that one can find in the class, and encodes also the
different types of symmetry groups.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:20:03 GMT"
},
{
"version": "v2",
"created": "Fri, 25 Jul 2008 12:03:56 GMT"
}
] | 2008-07-25T00:00:00 | [
[
"Fernandes",
"Rui Loja",
""
],
[
"Struchiner",
"Ivan",
""
]
] | [
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] |
712.3199 | Manuel Tessmer | M. Tessmer and A. Gopakumar | Gravitational waves from compact binaries inspiralling along
post-Newtonian accurate eccentric orbits: Data analysis implications | 12 pages, 3 figures, submitted to Phys. Rev. D | Phys.Rev.D78:084029,2008 | 10.1103/PhysRevD.78.084029 | null | gr-qc | null | Compact binaries inspiralling along eccentric orbits are plausible
gravitational wave (GW) sources for the ground-based laser interferometers. We
explore the losses in the event rates incurred when searching for GWs from
compact binaries inspiralling along post-Newtonian accurate eccentric orbits
with certain obvious non-optimal search templates. For the present analysis, GW
signals having 2.5 post-Newtonian accurate orbital evolution are modeled
following the phasing formalism, presented in [T. Damour, A. Gopakumar, and B.
R. Iyer, Phys. Rev. D \textbf{70}, 064028 (2004)]. We demonstrate that the
search templates that model in a gauge-invariant manner GWs from compact
binaries inspiralling under qudrupolar radiation reaction along 2PN accurate
circular orbits are very efficient in capturing our somewhat realistic GW
signals. However, three types of search templates based on the adiabatic,
complete adiabatic and gauge-dependent complete non-adiabatic approximants,
detailed in [P. Ajith, B. R. Iyer, C. A. K. Robinson and B. S. Sathyaprakash,
%``A new class of post-Newtonian approximants to the dynamics of inspiralling
%compact binaries: Test-mass in the Schwarzschild spacetime,'' Phys. Rev. D
{\bf 71}, 044029 (2005)], relevant for the circular inspiral under the
qudrupolar radiation reaction were found to be inefficient in capturing the
above mentioned eccentric signal. We conclude that further investigations will
be required to probe the ability of various types of PN accurate circular
templates, employed to analyze the LIGO/VIRGO data, to capture GWs from compact
binaries having tiny orbital eccentricities.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:21:08 GMT"
},
{
"version": "v2",
"created": "Fri, 23 May 2008 12:27:21 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Tessmer",
"M.",
""
],
[
"Gopakumar",
"A.",
""
]
] | [
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] |
712.32 | Laurene Jouve | L. Jouve and A.S. Brun (Laboratoire AIM, CEA/DSM-CNRS-Universit\'e
Paris Diderot, DAPNIA/SAp, France) | On the role of meridional flows in flux transport dynamo models | 12 pages, 10 ps figures | Astron.Astrophys.474:239-250,2007 | 10.1051/0004-6361:20077070 | null | astro-ph | null | The Sun is a magnetic star whose magnetism and cyclic activity is linked to
the existence of an internal dynamo. We aim to understand the establishment of
the solar magnetic 22-yr cycle, its associated butterfly diagram and field
parity selection through numerical simulations of the solar global dynamo.
Inspired by recent observations and 3D simulations that both exhibit
multicellular flows in the solar convection zone, we seek to characterise the
influence of various profiles of circulation on the behaviour of solar
mean-field dynamo models. We are using 2-D mean field flux transport
Babcock-Leighton numerical models in which we test several types of meridional
flows: 1 large single cell, 2 cells in radius and 4 cells per hemisphere. We
confirm that adding cells in latitude tends to speed up the dynamo cycle
whereas adding cells in radius more than triples the period. We find that the
cycle period in the four cells model is less sensitive to the flow speed than
in the other simpler meridional circulation profiles studied. Moreover, our
studies show that adding cells in radius or in latitude seems to favour the
parity switching to a quadrupolar solution. According to our numerical models,
the observed 22-yr cycle and dipolar parity is easily reproduced by models
including multicellular meridional flows. On the contrary, the resulting
butterfly diagram and phase relationship between the toroidal and poloidal
fields are affected to a point where it is unlikely that such multicellular
meridional flows persist for a long period of time inside the Sun, without
having to reconsider the model itself.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:32:59 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Jouve",
"L.",
"",
"Laboratoire AIM, CEA/DSM-CNRS-Université\n Paris Diderot, DAPNIA/SAp, France"
],
[
"Brun",
"A. S.",
"",
"Laboratoire AIM, CEA/DSM-CNRS-Université\n Paris Diderot, DAPNIA/SAp, France"
]
] | [
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] |
712.3201 | Pietro Falgari | P. Falgari | Four-fermion production near the W-pair production threshold | To appear in the proceedings of the 8th International Symposium on
Radiative Corrections, October 1-5, 2007, Florence, Italy | PoSRADCOR2007:003,2007 | null | PITHA 07/22, SFB/CPP-07-91 | hep-ph | null | I report on recent results for the total production cross section of the
process e- e+ -> mu- nubar_mu u dbar X near the W-pair production threshold up
to next-to-leading order in GammaW/MW alpha v^2 obtained in the framework of
unstable-particle effective field theory. Remaining theoretical uncertainties
and their impact on the experimental determination of the W mass are discussed.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:35:27 GMT"
}
] | 2009-04-14T00:00:00 | [
[
"Falgari",
"P.",
""
]
] | [
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] |
712.3202 | Megumi Harada | Megumi Harada, Paul Selick | Kirwan surjectivity in K-theory for Hamiltonian loop group quotients | 18 pages | null | null | null | math.SG math.AT | null | Let G be a compact Lie group and LG its associated loop group. The main
result of this manuscript is a surjectivity theorem from the equivariant
K-theory of a Hamiltonian LG-space onto the integral K-theory of its
Hamiltonian LG-quotient. Our result is a K-theoretic analogue of previous work
in rational Borel-equivariant cohomology of Bott, Tolman, and Weitsman. Our
proof techniques differ from that of Bott, Tolman, and Weitsman in that they
explicitly use the Borel construction, which we do not have at our disposal in
equivariant K-theory; we instead directly construct G-equivariant homotopy
equivalences to obtain the necessary isomorphisms in equivariant K-theory. The
main theorem should also be viewed as a first step toward a similar theorem in
K-theory for quasi-Hamiltonian G-spaces and their associated quasi-Hamiltonian
quotients.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:43:15 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Harada",
"Megumi",
""
],
[
"Selick",
"Paul",
""
]
] | [
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] |
712.3203 | Wan ChangLin | Changlin Wan, Zhongzhi Shi | Solving Medium-Density Subset Sum Problems in Expected Polynomial Time:
An Enumeration Approach | 11 pages, 1 figure | Changlin Wan, Zhongzhi Shi: Solving Medium-Density Subset Sum
Problems in Expected Polynomial Time: An Enumeration Approach. FAW 2008:
300-310 | 10.1007/978-3-540-69311-6_31 | null | cs.DS cs.CC cs.CR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The subset sum problem (SSP) can be briefly stated as: given a target integer
$E$ and a set $A$ containing $n$ positive integer $a_j$, find a subset of $A$
summing to $E$. The \textit{density} $d$ of an SSP instance is defined by the
ratio of $n$ to $m$, where $m$ is the logarithm of the largest integer within
$A$. Based on the structural and statistical properties of subset sums, we
present an improved enumeration scheme for SSP, and implement it as a complete
and exact algorithm (EnumPlus). The algorithm always equivalently reduces an
instance to be low-density, and then solve it by enumeration. Through this
approach, we show the possibility to design a sole algorithm that can
efficiently solve arbitrary density instance in a uniform way. Furthermore, our
algorithm has considerable performance advantage over previous algorithms.
Firstly, it extends the density scope, in which SSP can be solved in expected
polynomial time. Specifically, It solves SSP in expected $O(n\log{n})$ time
when density $d \geq c\cdot \sqrt{n}/\log{n}$, while the previously best
density scope is $d \geq c\cdot n/(\log{n})^{2}$. In addition, the overall
expected time and space requirement in the average case are proven to be
$O(n^5\log n)$ and $O(n^5)$ respectively. Secondly, in the worst case, it
slightly improves the previously best time complexity of exact algorithms for
SSP. Specifically, the worst-case time complexity of our algorithm is proved to
be $O((n-6)2^{n/2}+n)$, while the previously best result is $O(n2^{n/2})$.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:43:50 GMT"
},
{
"version": "v2",
"created": "Mon, 23 Jun 2008 02:00:12 GMT"
}
] | 2008-06-23T00:00:00 | [
[
"Wan",
"Changlin",
""
],
[
"Shi",
"Zhongzhi",
""
]
] | [
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] |
712.3204 | Francesco Giazotto | N. B. Kopnin, F. Taddei, J. P. Pekola, and F. Giazotto | Influence of photon-assisted tunneling on heat flow in a normal metal -
superconductor tunnel junction | 10 pages, 8 colour figures, published version | Phys. Rev. B 77, 104517 (2008) | 10.1103/PhysRevB.77.104517 | null | cond-mat.mes-hall cond-mat.supr-con | null | We have investigated theoretically the influence of an AC drive on heat
transport in a hybrid normal metal - superconductor tunnel junction in the
photon-assisted tunneling regime. We find that the useful heat flux out from
the normal metal is always reduced as compared to its magnitude under the
static and quasi-static drive conditions. Our results are useful to predict the
operative conditions of AC driven superconducting electron refrigerators.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:15:53 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Mar 2008 13:06:31 GMT"
}
] | 2008-03-21T00:00:00 | [
[
"Kopnin",
"N. B.",
""
],
[
"Taddei",
"F.",
""
],
[
"Pekola",
"J. P.",
""
],
[
"Giazotto",
"F.",
""
]
] | [
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] |
712.3205 | Ilia Zharkov | Ilia Zharkov | Tropical theta characteristics | 4 pages, still an addendum to math.AG/0612267v2, exposition improved,
description of positive theta added | null | null | null | math.AG math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This note is a follow up of math.AG/0612267v2 and it is largely inspired by a
beautiful description of Baker-Norine of non-effective degree (g-1) divisors
via chip-firing game. We consider the set of all theta characteristics on a
tropical curve and identify the Riemann constant as a unique non-effective one
among them.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 14:47:48 GMT"
},
{
"version": "v2",
"created": "Wed, 18 Feb 2009 22:33:45 GMT"
}
] | 2009-02-19T00:00:00 | [
[
"Zharkov",
"Ilia",
""
]
] | [
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712.3206 | Ram Brustein | Ram Brustein, Dan Gorbonos, Merav Hadad | Wald's entropy is equal to a quarter of the horizon area in units of the
effective gravitational coupling | 20 pages ; added clarifications, explanations, new section on the
choice of polarizations, results unchanged; replaced with published version | Phys.Rev.D79:044025,2009 | 10.1103/PhysRevD.79.044025 | null | hep-th gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Bekenstein-Hawking entropy of black holes in Einstein's theory of gravity
is equal to a quarter of the horizon area in units of Newton's constant. Wald
has proposed that in general theories of gravity the entropy of stationary
black holes with bifurcate Killing horizons is a Noether charge which is in
general different from the Bekenstein-Hawking entropy. We show that the Noether
charge entropy is equal to a quarter of the horizon area in units of the
effective gravitational coupling on the horizon defined by the coefficient of
the kinetic term of specific graviton polarizations on the horizon. We present
several explicit examples of static spherically symmetric black holes.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:13:40 GMT"
},
{
"version": "v2",
"created": "Wed, 12 Nov 2008 14:04:59 GMT"
},
{
"version": "v3",
"created": "Mon, 2 Mar 2009 12:04:01 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Brustein",
"Ram",
""
],
[
"Gorbonos",
"Dan",
""
],
[
"Hadad",
"Merav",
""
]
] | [
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] |
712.3207 | Monica Orienti | M. Orienti (1,2,3), D. Dallacasa (2,3),((1) IAC, (2) Dipartimento di
Astronomia, Bologna, (3) IRA-INAF, Bologna) | Constraining the nature of High Frequency Peakers. II. Polarization
properties | 9 pages, 2 figures; accepted for publication in A&A | null | 10.1051/0004-6361:20078572 | null | astro-ph | null | Aims: The ``bright'' High Frequency Peakers (HFPs) sample is a mixture of
blazars and intrinsically small and young radio sources. We investigate the
polarimetric characteristics of 45 High Frequency Peakers, from the ``bright''
HFP sample, in order to have a deeper knowledge of the nature of each object,
and to construct a sample made of genuine young radio sources only. Methods:
Simultaneous VLA observations carried out at 22.2, 15.3, 8.4 and 5.0 GHz,
together with the information at 1.4 GHz provided by the NVSS at an earlier
epoch, have been used to study the linearly polarized emission. Results: From
the analysis of the polarimetric properties of the 45 sources we find that 26
(58%) are polarized at least at one frequency, while 17 (38%) are completely
unpolarized at all frequencies. We find a correlation between fractional
polarization and the total intensity variability. We confirm that there is a
clear distinction between the polarization properties of galaxies and quasars:
17 (66%) quasars are highly polarized, while all the 9 galaxies are either
unpolarized (<0.2%) or marginally polarized with fractional polarization below
1%. This suggests that most HFP candidates identified with quasars are likely
to represent a radio source population different from young radio objects.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:14:07 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Orienti",
"M.",
""
],
[
"Dallacasa",
"D.",
""
]
] | [
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] |
712.3208 | Una Hwang | Una Hwang, Robert Petre, Kathryn A. Flanagan | X-ray Emitting Ejecta in Puppis A Observed with Suzaku | 25 pages latex, 6 postscript figures; ApJ, in press | null | 10.1086/528925 | null | astro-ph | null | We report the detection and localization of X-ray emitting ejecta in the
middle-aged Galactic supernova remnant Puppis A using five observations with
the Suzaku X-ray Imaging Spectrometer to survey the eastern and middle portions
of the remnant. A roughly 3' by 5', double-peaked region in the north center is
found to be highly enriched in Si and other elements relative to the rest of
the remnant. The X-ray fitted abundances are otherwise well below the solar
values. While the ejecta-enhanced regions show some variation of relative
element abundances, there is little evidence for a very strong enhancement of
one element over the others in the imaged portion of the remnant, except
possibly for a region of O and Ne enhancement in the remnant's south center.
There is no spatial correlation between the compact [O III] emitting ejecta
knots seen optically and the abundance enhancements seen in X-rays, although
they are located in the same vicinity. The map of fitted column density shows
strong variations across the remnant that echo earlier X-ray spectral hardness
maps. The ionization age (as fitted for single temperature models) is sharply
higher in a ridge behind the northeast-east boundary of the remnant, and is
probably related to the strong molecular cloud interaction along that boundary.
The temperature map, by comparison, shows relatively weak variations.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:21:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hwang",
"Una",
""
],
[
"Petre",
"Robert",
""
],
[
"Flanagan",
"Kathryn A.",
""
]
] | [
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] |
712.3209 | Hans-Joachim Drescher | H.J. Drescher (Frankfurt Institute for Advanced Studies), M. Strikman
(Pennsylvania State University) | Toward an effective centrality trigger in pp collisions at LHC | 4 pages, 6 figures | null | null | null | hep-ph | null | We investigate the impact of very strong small x gluon fields in colliding
nucleons at LHC energies on the interaction of valence quarks. We find that in
the range of small impact parameters, which contribute significantly to the
production of heavy new particles, several of the valence quarks receive large
transverse momenta, exceeding 1 GeV/c. This results in a suppression of leading
baryon production and consequently in an additional energy flow to smaller
rapidities. We suggest several triggers for centrality in pp collisions which
allow one to study the propagation of partons through gluon fields of a
strength comparable to the ones encountered in heavy ion collisions at the LHC.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:27:09 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Drescher",
"H. J.",
"",
"Frankfurt Institute for Advanced Studies"
],
[
"Strikman",
"M.",
"",
"Pennsylvania State University"
]
] | [
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] |
712.321 | Matthieu Marouby | Matthieu Marouby | Simulation of a Local Time Fractional Stable Motion | null | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper, we simulate sample paths of a class of symmetric
$\alpha$-stable processes using their series expression. We will develop a
result in the approximation of shot-noise series. And finally, we will get a
convergence rate for the approximation.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:28:55 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jul 2008 11:33:40 GMT"
}
] | 2008-07-16T00:00:00 | [
[
"Marouby",
"Matthieu",
""
]
] | [
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] |
712.3211 | Kirill Alekseev | Timo Hyart, Kirill N. Alekseev, and Erkki V. Thuneberg | Bloch gain in dc-ac-driven semiconductor superlattices in the absence of
electric domains | 13 pages, 12 figures | null | 10.1103/PhysRevB.77.165330 | null | cond-mat.mes-hall cond-mat.stat-mech | null | We study theoretically the feasibility of amplification and generation of
terahertz radiation in dc-ac-driven semiconductor superlattices in the absence
of electric domains. We find that if in addition to dc bias a strong THz pump
field is applied, Bloch gain profile for a small THz signal can be achieved
under conditions of positive static differential conductivity. Here the
positive differential conductivity arises, similarly to the case of
large-signal amplification scheme [H. Kroemer, cond-mat/0009311)], due to
modifications of dc current density caused by the application of high-frequency
ac field [K. Unterrainer \textit{et al.}, Phys. Rev. Lett. \textbf{76}, 2973
(1996)]. Whereas the sign of absorption at low and zero frequencies is
sensitive to the ac fields, the gain profile in the vicinity of gain maximum is
robust. We suggest to use this ac-induced effect in a starter for THz Bloch
oscillator. Our analysis demonstrates that the application of a short THz pulse
to a superlattice allows to suppress the undesirable formation of electric
domains and reach a sustained large-amplitude operation of the dc-biased Bloch
scillator.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:37:52 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hyart",
"Timo",
""
],
[
"Alekseev",
"Kirill N.",
""
],
[
"Thuneberg",
"Erkki V.",
""
]
] | [
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] |
712.3212 | Marten van Kerkwijk | M. H. van Kerkwijk (Toronto) and D. L. Kaplan (MIT) | Timing the Nearby Isolated Neutron Star RX J1856.5-3754 | 4 pages, 2 figures, 2 tables; accepted for publication in
Astrophysical Journal (Letters) | Astrophys.J.673:L163-L166, 2008 | 10.1086/528796 | null | astro-ph | null | RX J1856.5-3754 is the X-ray brightest among the nearby isolated neutron
stars. Its X-ray spectrum is thermal, and is reproduced remarkably well by a
black-body, but its interpretation has remained puzzling. One reason is that
the source did not exhibit pulsations, and hence a magnetic field
strength--vital input to atmosphere models--could not be estimated. Recently,
however, very weak pulsations were discovered. Here, we analyze these in
detail, using all available data from the XMM-Newton and Chandra X-ray
observatories. From frequency measurements, we set a 2-sigma upper limit to the
frequency derivative of \dot\nu<1.3e-14 Hz/s. Trying possible phase-connected
timing solutions, we find that one solution is far more likely than the others,
and we infer a most probable value of \dot\nu=(-5.98+/-0.14)e-16 Hz/s. The
inferred magnetic field strength is 1.5e13 G, comparable to what was found for
similar neutron stars. From models, the field seems too strong to be consistent
with the absence of spectral features for non-condensed atmospheres. It is
sufficiently strong, however, that the surface could be condensed, but only if
it is consists of heavy elements like iron. Our measurements imply a
characteristic age of about 4 Myr. This is longer than the cooling and
kinematic ages, as was found for similar objects, but at almost a factor ten,
the discrepancy is more extreme. A puzzle raised by our measurement is that the
implied rotational energy loss rate of about 3e30 erg/s is orders of magnitude
smaller than what was inferred from the H-alpha nebula surrounding the source.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:57:05 GMT"
}
] | 2010-04-30T00:00:00 | [
[
"van Kerkwijk",
"M. H.",
"",
"Toronto"
],
[
"Kaplan",
"D. L.",
"",
"MIT"
]
] | [
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712.3213 | John Irving | J. Irving and A. Rattan | The number of lattice paths below a cyclically shifting boundary | 20 pages, 13 figures | null | null | null | math.CO | null | We count the number of lattice paths lying under a cyclically shifting
piecewise linear boundary of varying slope. Our main result extends well known
enumerative formulae concerning lattice paths, and its derivation involves a
classical reflection argument. A refinement allows for the counting of paths
with a specified number of corners. We also apply the result to examine paths
dominated by periodic boundaries.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:48:31 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Irving",
"J.",
""
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[
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"A.",
""
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712.3214 | Mahir S. Hussein | M. S. Hussein, J. X. de Carvalho, M. P. Pato and A. J. Sargeant | Symmetry Breaking Study with Random Matrix Ensembles | 12 pages, 3 figures Contribution to the International Workshop on
Nuclei and Mesoscopic Physics (WNM07), 20-22 October, Michigan Sate
University, East Lansing, Michigan. To appear in a AIP Proceeding (Pawel
Danielewicz, Editor) | null | 10.1063/1.2915605 | null | physics.data-an | null | A random matrix model to describe the coupling of $m$-fold symmetry is
constructed. The particular threefold case is used to analyze data on
eigenfrequencies of elastomechanical vibration of an anisotropic quartz block.
It is suggested that such experimental/theoretical study may supply a powerful
means to discern intrinsic symmetry of physical systems.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:49:13 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hussein",
"M. S.",
""
],
[
"de Carvalho",
"J. X.",
""
],
[
"Pato",
"M. P.",
""
],
[
"Sargeant",
"A. J.",
""
]
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712.3215 | Francoise Sandoz-Guermond | Fran\c{c}oise Sandoz-Guermond (LIESP), Marc-Eric Bobiller-Chaumon
(GRePS) | L'accessibilit\'e des E-services aux personnes non-voyantes :
difficult\'es d'usage et recommandations | 4 pages | Dans International Conference Proceedings of IHM'2006 - IIHM :
Interaction Homme Machine, Montr\'eal : Canada (2006) | null | null | cs.HC | null | While taking into account handicapped people in the design of technologies
represents a social and political stake that becomes important (in particular
with the recent law on equal rights for all the citizens, March 2004), this
paper aims at evaluating the level of accessibility of two sites of E-services
thanks to tests of use and proposing a set of recommendations in order to
increase usability for the largest amount of people.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:54:07 GMT"
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] | 2007-12-20T00:00:00 | [
[
"Sandoz-Guermond",
"Françoise",
"",
"LIESP"
],
[
"Bobiller-Chaumon",
"Marc-Eric",
"",
"GRePS"
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] |
712.3216 | Benjamin Lungwitz | The NA49 Collaboration: B. Lungwitz, et al | Energy Dependence of Multiplicity Fluctuations in Heavy Ion Collisions
at the CERN SPS | 26 pages, 34 figures, updated version including referee comments | null | 10.1103/PhysRevC.78.034914 | null | nucl-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Multiplicity fluctuations of positively, negatively and all charged hadrons
in the forward hemisphere were studied in central Pb+Pb collisions at 20A, 30A,
40A, 80A and 158A GeV. The multiplicity distributions and their scaled
variances are presented in dependence of collision energy as well as of
rapidity and transverse momentum. The distributions have bell-like shape and
their scaled variances are in the range from 0.8 to 1.2 without any significant
structure in their energy dependence. No indication of the critical point in
fluctuations are observed. The string-hadronic model UrQMD significantly
overpredicts the mean, but approximately reproduces the scaled variance of the
multiplicity distributions. The predictions of the statistical hadron-resonance
gas model obtained within the grand-canonical and canonical ensembles disagree
with the measured scaled variances. The narrower than Poissonian multiplicity
fluctuations measured in numerous cases may be explained by the impact of
conservation laws on fluctuations in relativistic systems.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:02:17 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Jul 2008 14:14:36 GMT"
},
{
"version": "v3",
"created": "Sat, 9 Aug 2008 09:54:17 GMT"
}
] | 2013-05-29T00:00:00 | [
[
"The NA49 Collaboration",
"",
""
],
[
"Lungwitz",
"B.",
""
]
] | [
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712.3217 | Francois Delarue | Francois Delarue (PMA), Fr\'ed\'eric Lagouti\`ere (LJLL) | Probabilistic analysis of the upwind scheme for transport | null | Archive for Rational Mechanics and Analysis (2011) 229--268 | 10.1007/s00205-010-0322-x | null | math.NA math.PR | null | We provide a probabilistic analysis of the upwind scheme for
multi-dimensional transport equations. We associate a Markov chain with the
numerical scheme and then obtain a backward representation formula of
Kolmogorov type for the numerical solution. We then understand that the error
induced by the scheme is governed by the fluctuations of the Markov chain
around the characteristics of the flow. We show, in various situations, that
the fluctuations are of diffusive type. As a by-product, we prove that the
scheme is of order 1/2 for an initial datum in BV and of order 1/2-a, for all
a>0, for a Lipschitz continuous initial datum. Our analysis provides a new
interpretation of the numerical diffusion phenomenon.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:55:54 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Delarue",
"Francois",
"",
"PMA"
],
[
"Lagoutière",
"Frédéric",
"",
"LJLL"
]
] | [
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712.3218 | Matteo Luca Ruggiero | Matteo Luca Ruggiero | Gravitational Lensing and f(R) theories in the Palatini approach | 7 Pages, RevTex, 1 eps figure; references added; revised to match the
version accepted for publication in General Relativity and Gravitation | Gen.Rel.Grav.41:1497-1509,2009 | 10.1007/S1071400807172 10.1007/s10714-008-0717-2 | null | astro-ph gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate gravitational lensing in the Palatini approach to the f(R)
extended theories of gravity. Starting from an exact solution of the f(R) field
equations, which corresponds to the Schwarzschild-de Sitter metric and, on the
basis of recent studies on this metric, we focus on some lensing observables,
in order to evaluate the effects of the non linearity of the gravity
Lagrangian. We give estimates for some astrophysical events, and show that
these effects are tiny for galactic lenses, but become interesting for
extragalactic ones.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 15:57:55 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 16:26:42 GMT"
},
{
"version": "v3",
"created": "Mon, 3 Nov 2008 16:32:04 GMT"
}
] | 2009-07-22T00:00:00 | [
[
"Ruggiero",
"Matteo Luca",
""
]
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] |
712.3219 | Manfred Cuntz | W. von Bloh, C. Bounama, M. Cuntz, S. Franck | Habitability of Super-Earths: Gliese 581c and 581d | 3 pages, 1 figure; submitted to: Exoplanets: Detection, Formation and
Dynamics, IAU Symposium 249, eds. Y.-S. Sun, S. Ferraz-Mello, and J.-L. Zhou
(Cambridge: Cambridge University Press) | null | 10.1017/S1743921308017031 | null | astro-ph | null | The unexpected diversity of exoplanets includes a growing number of
super-Earth planets, i.e., exoplanets with masses smaller than 10 Earth masses.
Unlike the larger exoplanets previously found, these smaller planets are more
likely to have a similar chemical and mineralogical composition to the Earth.
We present a thermal evolution model for super-Earth planets to identify the
sources and sinks of atmospheric carbon dioxide. The photosynthesis-sustaining
habitable zone (pHZ) is determined by the limits of biological productivity on
the planetary surface. We apply our model to calculate the habitability of the
two super-Earths in the Gliese 581 system. The super-Earth Gl 581c is clearly
outside the pHZ, while Gl 581d is at the outer edge of the pHZ. Therefore it
could at least harbor some primitive forms of life.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:14:26 GMT"
},
{
"version": "v2",
"created": "Mon, 24 Dec 2007 20:05:08 GMT"
},
{
"version": "v3",
"created": "Fri, 15 Feb 2008 21:26:52 GMT"
},
{
"version": "v4",
"created": "Tue, 19 Feb 2008 22:16:26 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"von Bloh",
"W.",
""
],
[
"Bounama",
"C.",
""
],
[
"Cuntz",
"M.",
""
],
[
"Franck",
"S.",
""
]
] | [
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712.322 | Viviana Sica | Michael Gurstein | What is Community Informatics (and Why Does It Matter)? | 109 pages, ISBN 978-88-7699-097-7 (Printed edition), ISBN
978-88-7699-098-4 (Electronic edition), printed edition available at
http://www.amazon.com and on http://www.lulu.com | "Publishing studies" book series, edited by Giandomenico Sica,
ISSN 1973-6061 (Printed edition), ISSN 1973-6053 (Electronic edition) | null | null | cs.CY | null | Community Informatics (CI) is the application of information and
communications technologies (ICTs) to enable community processes and the
achievement of community objectives. CI goes beyond the "Digital Divide" to
making ICT access usable and useful to excluded populations and communities for
local economic development, social justice, and political empowerment. CI
approaches ICTs from a "community" perspective and develops strategies and
techniques for managing their use by communities both virtual and physical
including the variety of Community Networking applications. CI assumes that
both communities have characteristics, requirements, and opportunities that
require different strategies for ICT intervention and development from
individual access and use. Also, CI addresses ICT use in Developing Countries
as well as among the poor, the marginalized, the elderly, or those living in
remote locations in Developed Countries. CI is of interest both to ICT
practitioners and academic researchers and addresses the connections between
the policy and pragmatic issues arising from the tens of thousands of Community
Networks, Community Technology Centres, Telecentres, Community Communications
Centres, and Telecottages globally along with the rapidly emerging field of
electronically based virtual "communities".
Michael Gurstein, Ph.D. is Executive Director of the Centre for Community
Informatics Research, Development and Training (Vancouver BC), a Director of
The Information Society Institute, Cape Peninsula University of Technology,
Cape Town South Africa; and Research Professor in the School of Computer and
Information Systems at the New Jersey Institute of Technology, Newark.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:07:49 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Gurstein",
"Michael",
""
]
] | [
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] |
712.3221 | Jianguo Cao | Jianguo Cao, Bo Dai, Jiaqiang Mei | An optimal extension of Perelman's comparison theorem for quadrangles
and its applications | We corrected some inaccurate statements and definitions about
development maps related to Corollary 2.4, based on Professor Stephanie
Alexander's suggestions | null | null | null | math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this paper we discuss an extension of Perelman's comparison for
quadrangles. Among applications of this new comparison theorem, we study the
equidistance evolution of hypersurfaces in Alexandrov spaces with non-negative
curvature. We show that, in certain cases, the equidistance evolution of
hypersurfaces become totally convex relative to a bigger sub-domain. An optimal
extension of 2nd variational formula for geodesics by Petrunin will be derived
for the case of non-negative curvature.
In addition, we also introduced the generalized second fundament forms for
subsets in Alexandrov spaces. Using this new notion, we will propose an
approach to study two open problems in Alexandrov geometry.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:08:35 GMT"
},
{
"version": "v2",
"created": "Fri, 3 Apr 2009 17:57:00 GMT"
}
] | 2009-04-03T00:00:00 | [
[
"Cao",
"Jianguo",
""
],
[
"Dai",
"Bo",
""
],
[
"Mei",
"Jiaqiang",
""
]
] | [
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712.3222 | Anna Aret | A. Sapar, A. Aret, L. Sapar, R. Poolam\"ae | A Pan-Spectral Method of Abundance Determination | 4 pages, 2 figures, contribution presented at the ESO/Lisbon/Aveiro
Workshop on Precision Spectroscopy in Astrophysics held in Aveiro, Portugal,
11-15 September 2006 | In: Precision Spectroscopy in Astrophysics, ESO Astrophysics
Symposia, Springer 2008, 145-148 | 10.1007/978-3-540-75485-5_32 | null | astro-ph | null | We propose a new method for determination of element abundances in stellar
atmospheres aimed for the automatic processing of high-quality stellar spectra.
The pan-spectral method is based on weighted cumulative line-widths Q of
studied element. Difference in quantities Q found from synthetic and observed
spectra gives a correction to the initial abundance. Final abundances are then
found by rapidly converging iterations. Calculations can be made for many
elements simultaneously and do not demand supercomputers.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:12:50 GMT"
}
] | 2012-04-02T00:00:00 | [
[
"Sapar",
"A.",
""
],
[
"Aret",
"A.",
""
],
[
"Sapar",
"L.",
""
],
[
"Poolamäe",
"R.",
""
]
] | [
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] |
712.3223 | Pedro Jesus Salas | Pedro J. Salas | Simple fault-tolerant encoding over q-ary CSS quantum codes | null | Int. Journal of Quantum Information 5 (2007) 705-716 | null | null | quant-ph | null | CSS codes are a subfamily of stabilizer codes especially appropriate for
fault-tolerant quantum computations. A very simple method is proposed to encode
a general qudit when a Calderbank-Shor-Steane quantum code, defined over a
q-ary alphabet, is used.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:14:37 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Salas",
"Pedro J.",
""
]
] | [
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712.3224 | Anastasios Avgoustidis | A. Avgoustidis | Cosmic String Dynamics and Evolution in Warped Spacetime | 21 pages, 5 figures; Discussion section expanded, physical
implications further explored; To appear in PRD | Phys.Rev.D78:023501,2008 | 10.1103/PhysRevD.78.023501 | UB-ECM-PF-07/35, DAMTP-2007-121 | hep-th astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study the dynamics and evolution of Nambu-Goto strings in a warped
spacetime, where the warp factor is a function of the internal coordinates
giving rise to a `throat' region. The microscopic equations of motion for
strings in this background include potential and friction terms, which attract
the strings towards the bottom of the warping throat. However, by considering
the resulting macroscopic equations for the velocities of strings in the
vicinity of the throat, we note the absence of enough classical damping to
guarantee that the strings actually reach the warped minimum and stabilise
there. Instead, our classical analysis supports a picture in which the strings
experience mere deflections and bounces around the tip, rather than strongly
damped oscillations. Indeed, 4D Hubble friction is inefficient in the internal
dimensions and there is no other classical mechanism known, which could provide
efficient damping. These results have potentially important implications for
the intercommuting probabilities of cosmic superstrings.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:15:10 GMT"
},
{
"version": "v2",
"created": "Wed, 11 Jun 2008 15:05:10 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Avgoustidis",
"A.",
""
]
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] |
712.3225 | Thomas B. Bahder | Paul A. Lopata, Thomas B. Bahder | Fishing for Eavesdroppers | 21 pages, 1 figure. Submitted to Quantum Information & Computation
journal | null | null | null | quant-ph | null | A method is given to detect the presence of eavesdroppers when a noisy
message is sent to a privileged receiver. A proof of the effectiveness if this
method is demonstrated, and a comparison is made to other quantum cryptographic
tasks.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:21:40 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 17:52:38 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Lopata",
"Paul A.",
""
],
[
"Bahder",
"Thomas B.",
""
]
] | [
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] |
712.3226 | Harvey S. Reall | Harvey S. Reall | Counting the microstates of a vacuum black ring | 7 pages | JHEP0805:013,2008 | 10.1088/1126-6708/2008/05/013 | null | hep-th | null | The Bekenstein-Hawking entropy of an extremal vacuum black ring is derived
from a microscopic counting of states. The entropy of extremal Kaluza-Klein
black holes with ergospheres is also derived.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:32:35 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Reall",
"Harvey S.",
""
]
] | [
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] |
712.3227 | Thomas Schulte-Herbr\"uggen | T. Schulte-Herbrueggen, A. Spoerl, and S.J. Glaser | Quantum CISC Compilation by Optimal Control and Scalable Assembly of
Complex Instruction Sets beyond Two-Qubit Gates | substantially enlarged update with new sections; 19 pages, 17
figures; comments welcome | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a quantum CISC compiler and show how to assemble complex
instruction sets in a scalable way. Enlarging the toolbox of universal gates by
optimised complex multi-qubit instruction sets thus paves the way to fight
decoherence for realistic settings.
Compiling a quantum module into the machine code for steering a concrete
quantum hardware device lends itself to be tackled by means of optimal quantum
control. To this end, there are two opposite approaches: (i) one may use a
decomposition into the restricted instruction set (RISC) of universal one- and
two-qubit gates, which in turn have prefabricated translations into the machine
code or (ii) one may prefer to generate the entire target module directly by a
complex instruction set (CISC) of available controls. Here we advocate direct
compilation up to the limit of system size a classical high-performance
parallel computer cluster can reasonably handle. For going beyond these limits,
i.e. for large systems we propose a combined way, namely (iii) to make
recursive use of medium-sized building blocks generated by optimal control in
the sense of a quantum CISC compiler.
The advantage of the method over standard RISC compilations into one- and
two-qubit universal gates is explored on the parallel cluster HLRB-II (with a
total LINPACK performance of 63.3 TFlops/s) for the quantum Fourier transform,
the indirect SWAP gate as well as for multiply-controlled CNOT gates.
Implications for upper limits to time complexities are also derived.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:31:26 GMT"
},
{
"version": "v2",
"created": "Mon, 22 Dec 2008 17:39:41 GMT"
}
] | 2008-12-22T00:00:00 | [
[
"Schulte-Herbrueggen",
"T.",
""
],
[
"Spoerl",
"A.",
""
],
[
"Glaser",
"S. J.",
""
]
] | [
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] |
712.3228 | Chris Sneden | Ian B. Thompson, Inese I. Ivans, Sara Bisterzo, Christopher Sneden,
Roberto Gallino, Sylvie Vauclair, Gregory S. Burley, Stephen A. Shectman,
George W. Preston | CS22964-161: A Double-Lined Carbon- and s-Process-Enhanced Metal-Poor
Binary Star | manuscript, 7 tables, 13 figures. ApJ, in press | null | 10.1086/529016 | null | astro-ph | null | A detailed high-resolution spectroscopic analysis is presented for the
carbon-rich low metallicity Galactic halo object CS 22964-161. We have
discovered that CS 22964-161 is a double-lined spectroscopic binary, and have
derived accurate orbital components for the system. From a model atmosphere
analysis we show that both components are near the metal-poor main-sequence
turnoff. Both stars are very enriched in carbon and in neutron-capture elements
that can be created in the s-process, including lead. The primary star also
possesses an abundance of lithium close to the value of the ``Spite-Plateau''.
The simplest interpretation is that the binary members seen today were the
recipients of these anomalous abundances from a third star that was losing mass
as part of its AGB evolution. We compare the observed CS 22964-161 abundance
set with nucleosynthesis predictions of AGB stars, and discuss issues of
envelope stability in the observed stars under mass transfer conditions, and
consider the dynamical stability of the alleged original triple star. Finally,
we consider the circumstances that permit survival of lithium, whatever its
origin, in the spectrum of this extraordinary system.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:36:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Thompson",
"Ian B.",
""
],
[
"Ivans",
"Inese I.",
""
],
[
"Bisterzo",
"Sara",
""
],
[
"Sneden",
"Christopher",
""
],
[
"Gallino",
"Roberto",
""
],
[
"Vauclair",
"Sylvie",
""
],
[
"Burley",
"Gregory S.",
""
],
[
"Shectman",
"Stephen A.",
""
],
[
"Preston",
"George W.",
""
]
] | [
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] |
712.3229 | Luen-Chau Li | Luen-Chau Li | Long time behaviour for a class of low-regularity solutions of the
Camassa-Holm equation | 30 pages | Commun. Math. Phys. 285, 265-291 (2009) | 10.1007/s00220-008-0603-5 | null | math-ph math.MP math.SP | null | In this paper, we investigate the long time behaviour for a class of
low-regularity solutions of the Camassa-Holm equation given by the
superposition of infinitely many interacting traveling waves with corners at
their peaks.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:39:04 GMT"
}
] | 2010-07-23T00:00:00 | [
[
"Li",
"Luen-Chau",
""
]
] | [
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712.323 | Jan Draisma | Jan Draisma and Jochen Kuttler | On the ideals of equivariant tree models | 23 pages. Greatly improved exposition, in part following suggestions
by a referee--thanks! Also added example | Mathematische Annalen 344(3):619-644, 2009 | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We introduce equivariant tree models in algebraic statistics, which unify and
generalise existing tree models such as the general Markov model, the strand
symmetric model, and group based models. We focus on the ideals of such models.
We show how the ideals for general trees can be determined from the ideals for
stars. The main novelty is our proof that this procedure yields the entire
ideal, not just an ideal defining the model set-theoretically. A corollary of
theoretical importance is that the ideal for a general tree is generated by the
ideals of its flattenings at vertices.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:46:31 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 10:24:00 GMT"
},
{
"version": "v3",
"created": "Thu, 21 Aug 2008 15:34:59 GMT"
}
] | 2017-10-10T00:00:00 | [
[
"Draisma",
"Jan",
""
],
[
"Kuttler",
"Jochen",
""
]
] | [
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712.3231 | Olivier Wintenberger | Paul Doukhan (CREST, CES), Olivier Wintenberger (CES, SAMOS) | Weakly dependent chains with infinite memory | Stochastic Processes and their Applications (2008) accept\'e | null | null | null | math.PR math.ST stat.TH | null | We prove the existence of a weakly dependent strictly stationary solution of
the equation $ X_t=F(X_{t-1},X_{t-2},X_{t-3},...;\xi_t)$ called {\em chain with
infinite memory}. Here the {\em innovations} $\xi_t$ constitute an independent
and identically distributed sequence of random variables. The function $F$
takes values in some Banach space and satisfies a Lipschitz-type condition. We
also study the interplay between the existence of moments and the rate of decay
of the Lipschitz coefficients of the function $F$. With the help of the weak
dependence properties, we derive Strong Laws of Large Number, a Central Limit
Theorem and a Strong Invariance Principle.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:47:55 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Doukhan",
"Paul",
"",
"CREST, CES"
],
[
"Wintenberger",
"Olivier",
"",
"CES, SAMOS"
]
] | [
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] |
712.3232 | Vassilios Zamarias | Bertha Cuadros-Melgar, Eleftherios Papantonopoulos, Minas Tsoukalas,
Vassilios Zamarias | String-Like BTZ on Codimension-2 Braneworlds in the Thin Brane Limit | Title changed, reference added, shortened to match the published
version in Physical Review Letters | Phys.Rev.Lett.100:221601,2008 | 10.1103/PhysRevLett.100.221601 | null | hep-th astro-ph gr-qc | null | We consider five-dimensional gravity with a Gauss-Bonnet term in the bulk and
an induced gravity term on a 2-brane of codimension-2. We show that this system
admits BTZ black holes on the 2-brane which are extended into the bulk with
regular horizons.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:56:35 GMT"
},
{
"version": "v2",
"created": "Sun, 4 May 2008 19:00:28 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Cuadros-Melgar",
"Bertha",
""
],
[
"Papantonopoulos",
"Eleftherios",
""
],
[
"Tsoukalas",
"Minas",
""
],
[
"Zamarias",
"Vassilios",
""
]
] | [
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] |
712.3233 | Anton Akhmerov R | A. R. Akhmerov, J. H. Bardarson, A. Rycerz, C. W. J. Beenakker | Theory of the valley-valve effect in graphene nanoribbons | 5 pages, 6 figures, v3 added more numerical data and an appendix with
details of the calculation | Phys. Rev. B 77, 205416 (2008) | 10.1103/PhysRevB.77.205416 | null | cond-mat.mes-hall | null | A potential step in a graphene nanoribbon with zigzag edges is shown to be an
intrinsic source of intervalley scattering -- no matter how smooth the step is
on the scale of the lattice constant a. The valleys are coupled by a pair of
localized states at the opposite edges, which act as an attractor/repellor for
edge states propagating in valley K/K'. The relative displacement Delta along
the ribbon of the localized states determines the conductance G. Our result
G=(e^{2}/h)[1-\cos(N\pi+2\pi\Delta/3a)] explains why the ``valley-valve''
effect (the blocking of the current by a p-n junction) depends on the parity of
the number N of carbon atoms across the ribbon.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 16:55:05 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Apr 2008 19:59:34 GMT"
},
{
"version": "v3",
"created": "Thu, 17 Apr 2008 20:26:23 GMT"
}
] | 2015-10-12T00:00:00 | [
[
"Akhmerov",
"A. R.",
""
],
[
"Bardarson",
"J. H.",
""
],
[
"Rycerz",
"A.",
""
],
[
"Beenakker",
"C. W. J.",
""
]
] | [
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712.3234 | Rahim Moosa | Rahim Moosa, Ruxandra Moraru, and Matei Toma | An essentially saturated surface not of Kaehler-type | 10 pages | null | 10.1112/blms/bdn063 | null | math.CV math.LO | null | It is shown that if $X$ is an Inoue surface of type $S_M$ then the
irreducible components of the Douady space of $X^n$ are compact, for all $n>0$.
This gives an example of an essentially saturated compact complex manifold (in
the sense of model theory) that is not of Kaehler-type. Among the known compact
complex surfaces without curves, it is shown that these are the only examples.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:02:00 GMT"
}
] | 2014-02-26T00:00:00 | [
[
"Moosa",
"Rahim",
""
],
[
"Moraru",
"Ruxandra",
""
],
[
"Toma",
"Matei",
""
]
] | [
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] |
712.3235 | Andrew Callister | Andrew K. Callister and Douglas J. Smith | Topological BPS charges in 10 and 11-dimensional supergravity | 64 pages, no figures, references added | Phys.Rev.D78:065042,2008 | 10.1103/PhysRevD.78.065042 | null | hep-th | null | We consider the supersymmetry algebras of the 10 and 11 dimensional maximal
supergravities. We construct expressions from which the topological charge
structure of the algebras can be determined in supersymmetric curved
backgrounds. These are interpreted as the topological charges of the 1/2-BPS
states that are found in the theories. We consider charges for all the M-, NS-
and D-branes as well as the Kaluza Klein monopoles. We also show that the
dimensional reduction relations between the 11-d and IIA charges, and T-duality
relations of the IIA and IIB charges match those found for the branes
themselves. Finally we consider the massive versions of the IIA and 11-d
theories and find that the expressions for the charges, with a slight
modification, are still valid in those instances.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:07:31 GMT"
},
{
"version": "v2",
"created": "Tue, 1 Apr 2008 15:27:24 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Callister",
"Andrew K.",
""
],
[
"Smith",
"Douglas J.",
""
]
] | [
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712.3236 | Achamveedu Gopakumar | Achamveedu Gopakumar | New Class of Gravitational Wave Templates for Inspiralling Compact
Binaries | 5 pages | null | null | null | gr-qc | null | Compact binaries inspiralling along quasi-circular orbits are the most
plausible gravitational wave (GW) sources for the operational, planned and
proposed laser interferometers. We provide new class of restricted
post-Newtonian accurate GW templates for non-spinning compact binaries
inspiralling along PN accurate quasi-circular orbits. Arguments based on data
analysis, theoretical and astrophysical considerations are invoked to show why
these time-domain Taylor approximants should be interesting to various GW data
analysis communities.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:14:33 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Gopakumar",
"Achamveedu",
""
]
] | [
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712.3237 | Kiril Datchev | Kiril Datchev | Local smoothing for scattering manifolds with hyperbolic trapped sets | 16 pages. Published version available at
http://www.springerlink.com/content/r663321331243288/?p=5ad2fe4778a742e4949de2030a409358&pi=11 | Communications in Mathematical Physics, Vol. 286, No. 3, pp.
837-850, 2009 | 10.1007/s00220-008-0684-1 | null | math.AP math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove a resolvent estimate for the Laplace-Beltrami operator on a
scattering manifold with a hyperbolic trapped set, and as a corollary deduce
local smoothing. We use a result of Nonnenmacher-Zworski to provide an estimate
near the trapped region, a result of Burq and Cardoso-Vodev to provide an
estimate near infinity, and the microlocal calculus on scattering manifolds to
combine the two.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:18:13 GMT"
},
{
"version": "v2",
"created": "Wed, 27 Aug 2008 20:01:27 GMT"
},
{
"version": "v3",
"created": "Thu, 29 Jan 2009 21:15:41 GMT"
}
] | 2012-06-06T00:00:00 | [
[
"Datchev",
"Kiril",
""
]
] | [
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712.3238 | Jeffrey C. Lagarias | Jeffrey C Lagarias | The Schr\"odinger operator with Morse potential on the right half line | 33 pages; v2 and v3 introduction revised, Polya and other refs.
added, v4,v5 intro revised, typos corrected, v6 corrections to some details | Communications in Number Theory and Physics 3 (2009), No.2,
323--361 | null | null | math.SP math-ph math.MP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This paper studies the Schr\"odinger operator with Morse potential on a right
half line [u, \infty) and determines the Weyl asymptotics of eigenvalues for
constant boundary conditions. It obtains information on zeros of the Whittaker
function $W_{\kappa, \mu}(x)$ for fixed real parameters $\kappa, x$, with x
positive, viewed as an entire function of the complex variable $\mu$. In this
case all zeros lie on the imaginary axis, with the exception, if $k<0$, of a
finite number of real zeros. We obtain an asymptotic formula for the number of
zeros of modulus at most T of form $N(T) = (2/\pi) T \log T + f(u) T + O(1)$.
Some parallels are noted with zeros of the Riemann zeta function.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:25:42 GMT"
},
{
"version": "v2",
"created": "Tue, 11 Nov 2008 19:15:09 GMT"
},
{
"version": "v3",
"created": "Tue, 16 Dec 2008 03:30:17 GMT"
},
{
"version": "v4",
"created": "Thu, 18 Dec 2008 19:59:12 GMT"
},
{
"version": "v5",
"created": "Fri, 26 Jun 2009 19:54:48 GMT"
},
{
"version": "v6",
"created": "Tue, 18 Aug 2009 19:21:10 GMT"
}
] | 2010-12-09T00:00:00 | [
[
"Lagarias",
"Jeffrey C",
""
]
] | [
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] |
712.3239 | Manfred Cuntz | J. Eberle, M. Cuntz, Z. E. Musielak | Orbital Stability of Planets in Binary Systems: A New Look at Old
Results | 3 pages, 1 figure; submitted to: Exoplanets: Detection, Formation and
Dynamics, IAU Symposium 249, eds. Y.-S. Sun, S. Ferraz-Mello, and J.-L. Zhou
(Cambridge: Cambridge University Press) | null | 10.1017/S1743921308017043 | null | astro-ph | null | About half of all known stellar systems with Sun-like stars consist of two or
more stars, significantly affecting the orbital stability of any planet in
these systems. This observational evidence has prompted a large array of
theoretical research, including the derivation of mathematically stringent
criteria for the orbital stability of planets in stellar binary systems, valid
for the "coplanar circular restricted three-body problem". In the following, we
use these criteria to explore the validity of results from previous theoretical
studies.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:03:55 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 21:17:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Eberle",
"J.",
""
],
[
"Cuntz",
"M.",
""
],
[
"Musielak",
"Z. E.",
""
]
] | [
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] |
712.324 | Ryan Gutenkunst | Ryan N. Gutenkunst and James P. Sethna | Adaptive mutation of biochemical reaction constants: Fisher's
geometrical model without pleiotropy | 9 pages, 4 figures, submitted | null | null | LA-UR: 10-04348 | q-bio.PE | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The distribution of fitness effects of adaptive mutations remains poorly
understood, both empirically and theoretically. We study this distribution
using a version of Fisher's geometrical model without pleiotropy, such that
each mutation affects only a single trait. We are motivated by the notion of an
organism's chemotype, the set of biochemical reaction constants that govern its
molecular constituents. From physical considerations, we expect the chemotype
to be of high dimension and to exhibit very little pleiotropy. Our model
generically predicts striking cusps in the distribution of the fitness effects
of arising and fixed mutations. It further predicts that a single element of
the chemotype should comprise all mutations at the high-fitness ends of these
distributions. Using extreme value theory, we show that the two cusps with the
highest fitnesses are typically well-separated, even when the chemotype
possesses thousands of elements; this suggests a means to observe these cusps
experimentally. More broadly, our work demonstrates that new insights into
evolution can arise from the chemotype perspective, a perspective between the
genotype and the phenotype.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:20:28 GMT"
},
{
"version": "v2",
"created": "Mon, 28 Jun 2010 20:12:19 GMT"
}
] | 2015-03-13T00:00:00 | [
[
"Gutenkunst",
"Ryan N.",
""
],
[
"Sethna",
"James P.",
""
]
] | [
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] |
712.3241 | Efrat Shimshoni | G. Venketeswara Pai, E. Shimshoni and N. Andrei | Resistivity of Inhomogeneous Superconducting Wires | 10 pages, 3 colored figures | Phys. Rev. B 77, 104528 (2008). | null | null | cond-mat.supr-con cond-mat.str-el | null | We study the contribution of quantum phase fluctuations in the
superconducting order parameter to the low--temperature resistivity $\rho(T)$
of a dirty and inhomogeneous superconducting wire. In particular, we account
for random spatial fluctuations of arbitrary size in the wire thickness. For a
typical wire thickness above the critical value for superconductor--insulator
transition, phase--slips processes can be treated perturbatively. We use a
memory formalism approach, which underlines the role played by weak violation
of conservation laws in the mechanism for generating finite resistivity. Our
calculations yield an expression for $\rho(T)$ which exhibits a smooth
crossover from a homogeneous to a ``granular'' limit upon increase of $T$,
controlled by a ``granularity parameter'' $D$ characterizing the size of
thickness fluctuations. For extremely small $D$, we recover the power--law
dependence $\rho(T)\sim T^\alpha$ obtained by unbinding of quantum
phase--slips. However in the strongly inhomogeneous limit, the exponent
$\alpha$ is modified and the prefactor is {\em exponentially enhanced}. We
examine the dependence of the exponent $\alpha$ on an external magnetic field
applied parallel to the wire. Finally, we show that the power--law dependence
at low $T$ is consistent with a series of experimental data obtained in a
variety of long and narrow samples. The values of $\alpha$ extracted from the
data, and the corresponding field dependence, are consistent with known
parameters of the corresponding samples.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:32:47 GMT"
}
] | 2009-01-27T00:00:00 | [
[
"Pai",
"G. Venketeswara",
""
],
[
"Shimshoni",
"E.",
""
],
[
"Andrei",
"N.",
""
]
] | [
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] |
712.3242 | Daniel Sudarsky | Daniel Sudarsky | Unspeakables and the Epistemological path towards Quantum Gravity | Invited article for "GRF2007 Special Issue of " IJMPD . In press | Int.J.Mod.Phys.D17:425-443,2008 | 10.1142/S0218271808012103 | null | gr-qc | null | We offer a critical assessment of some generic features of various of the
current approaches towards the construction of a Theory of Quantum Gravity. We
will argue that there is a need for further conceptual clarifications before
such an enterprise can be launched on a truly well grounded setting, and that
one of the guiding principles that can be viewed as part of the reasons for
successes of the past theoretical developments is the identification of
Unspeakables: Concepts that should not only play no role in the formulation of
the theories, but ones that the formalism of the theory itself should prevent
from ever been spoken about.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:35:29 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Sudarsky",
"Daniel",
""
]
] | [
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712.3243 | Nathan M. Dunfield | Nathan M. Dunfield and Dinakar Ramakrishnan | Increasing the number of fibered faces of arithmetic hyperbolic
3-manifolds | 42 pages, 7 figures; V2: minor improvements, to appear in Amer. J.
Math | Amer. J. Math 132 (2010), 53-97 | 10.1353/ajm.0.0098 | null | math.GT math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We exhibit a closed hyperbolic 3-manifold which satisfies a very strong form
of Thurston's Virtual Fibration Conjecture. In particular, this manifold has
finite covers which fiber over the circle in arbitrarily many ways. More
precisely, it has a tower of finite covers where the number of fibered faces of
the Thurston norm ball goes to infinity, in fact faster than any power of the
logarithm of the degree of the cover, and we give a more precise quantitative
lower bound. The example manifold M is arithmetic, and the proof uses detailed
number-theoretic information, at the level of the Hecke eigenvalues, to drive a
geometric argument based on Fried's dynamical characterization of the fibered
faces. The origin of the basic fibration of M over the circle is the modular
elliptic curve E=X_0(49), which admits multiplication by the ring of integers
of Q[sqrt(-7)]. We first base change the holomorphic differential on E to a
cusp form on GL(2) over K=Q[sqrt(-3)], and then transfer over to a quaternion
algebra D/K ramified only at the primes above 7; the fundamental group of M is
a quotient of the principal congruence subgroup of level 7 of the
multiplicative group of a maximal order of D. To analyze the topological
properties of M, we use a new practical method for computing the Thurston norm,
which is of independent interest. We also give a non-compact finite-volume
hyperbolic 3-manifold with the same properties by using a direct topological
argument.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:37:24 GMT"
},
{
"version": "v2",
"created": "Tue, 16 Dec 2008 19:54:19 GMT"
}
] | 2010-06-01T00:00:00 | [
[
"Dunfield",
"Nathan M.",
""
],
[
"Ramakrishnan",
"Dinakar",
""
]
] | [
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] |
712.3244 | Prabir Pal | M. Chakraborty, P. Pal and B. R. Sekhar | Half Metallicity in Pr$_{0.75}$Sr$_{0.25}$MnO$_3$: A first Principle
study | 8 pages, 3 figures | Solid State Communications 145 (2008) 197-200 | 10.1016/j.ssc.2007.10.025 | null | cond-mat.str-el cond-mat.mtrl-sci | null | In this communication we present a first principle study of
Pr$_{1-x}$Sr$_{x}$MnO$_3$ with $x = 0.25$. While the parent compounds of this
system are antiferromagnetic insulators with different structural and magnetic
ground states, the $x = 0.25$ is in the colossal magnetoresistance regime of
the Pr$_{1-x}$Sr$_{x}$MnO$_3$ phase diagram [C. Martin, A. Maignan, M. Hervieu,
B. Raveau, Phys. Rev. B 60 (1999) 12191]. Our band structure calculations for
the end-point compounds matches well with the existing theoretical and
experimental results [C. Martin, A. Maignan, M. Hervieu, B. Raveau, Phys. Rev.
B 60 (1999) 12191; Rune Sondena, P. Ravindran, Svein Stolen, Tor Grande,
Michael Hanfland, Phys. Rev. B 74 (2006) 144102]. Interestingly, our
calculations show that the Pr$_{0.75}$Sr$_{0.25}$MnO$_3$ has a half-metallic
character with a huge band gap of 2.8 eV in the minority band. We believe this
result would fuel further interest in some of these special compositions of
colossal magnetoresistive manganites as they could be potential candidates for
spintronic devices. We discuss the half-metallicity of the
Pr$_{0.75}$Sr$_{0.25}$MnO$_3$ in the light of changes in the orbital
hybridization as a result of Sr doping in PrMnO$_3$. Further, we highlight the
importance of half-metallicity for a consolidated understanding of colossal
magnetoresistance effect.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:38:29 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Chakraborty",
"M.",
""
],
[
"Pal",
"P.",
""
],
[
"Sekhar",
"B. R.",
""
]
] | [
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] |
712.3245 | Denis I. Borisov | Denis Borisov and Pedro Freitas | Singular asymptotic expansions for Dirichlet eigenvalues and
eigenfunctions of the Laplacian on thin planar domains | null | null | null | null | math.SP math-ph math.MP | null | We consider the Laplace operator with Dirichlet boundary conditions on a
planar domain and study the effect that performing a scaling in one direction
has on the spectrum. We derive the asymptotic expansion for the eigenvalues and
corresponding eigenfunctions as a function of the scaling parameter around
zero. This method allows us, for instance, to obtain an approximation for the
first Dirichlet eigenvalue for a large class of planar domains, under very mild
assumptions.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:40:27 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Borisov",
"Denis",
""
],
[
"Freitas",
"Pedro",
""
]
] | [
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] |
712.3246 | Remo Garattini | Remo Garattini | Extracting the Cosmological Constant from the Wheeler DeWitt Equation in
a Modified Gravity Theory | Talk given at QFEXT 07, Workshop on Quantum Field Theory Under the
Influence of External Conditions, Leipzig, 17-21 Sep 2007 and talk given at
9th International Conference on Path Integrals - New Trends and Perspectives,
Dresden, 23-28 September 2007. 8 pages, accepted for publication in Journal
of Physics A | J.Phys.A41:164057,2008 | 10.1088/1751-8113/41/16/164057 | null | gr-qc hep-th | null | We discuss how to extract information about the cosmological constant from
the Wheeler-DeWitt equation, considered as an eigenvalue of a Sturm-Liouville
problem. A generalization to a f(R)theory is taken under examination. The
equation is approximated to one loop with the help of a variational approach
with Gaussian trial wave functionals. We use a zeta function regularization to
handle with divergences. A renormalization procedure is introduced to remove
the infinities together with a renormalization group equation.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 18:03:26 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Garattini",
"Remo",
""
]
] | [
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] |
712.3247 | Tomasz Dietl | Hideo Ohno and Tomasz Dietl | Spin-transfer physics and the model of ferromagnetism in (Ga,Mn)As | 13 pages, 1 figure, to be published in J. Magn. Magn. Materials,
section "Current Perspectives" | J. Magn. Magn. Mat. 320 (2008) 1293--1299 | 10.1016/j.jmmm.2007.12.016 | null | cond-mat.mtrl-sci cond-mat.str-el | null | We describe recent progress and open questions in the physics of
current-induced domain-wall displacement and creep in (Ga,Mn)As. Furthermore,
the reasons are recalled why, despite strong disorder and localization, the p-d
Zener model is suitable for the description of this system.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:55:50 GMT"
}
] | 2013-11-15T00:00:00 | [
[
"Ohno",
"Hideo",
""
],
[
"Dietl",
"Tomasz",
""
]
] | [
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] |
712.3248 | Fabio Perroni | Samuel Boissiere, Etienne Mann, Fabio Perroni | The cohomological crepant resolution conjecture for P(1,3,4,4) | 11 pages, 1 figure | null | null | null | math.AG | null | We prove the cohomological crepant resolution conjecture of Ruan for the
weighted projective space P(1,3,4,4). To compute the quantum corrected
cohomology ring we combine the results of Coates-Corti-Iritani-Tseng on
P(1,1,1,3) and our previous results.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 17:57:23 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Boissiere",
"Samuel",
""
],
[
"Mann",
"Etienne",
""
],
[
"Perroni",
"Fabio",
""
]
] | [
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] |
712.3249 | Stephan Schulz | Stephan Schulz, Ulrich Poschinger, Frank Ziesel, and Ferdinand
Schmidt-Kaler | Sideband cooling and coherent dynamics in a microchip multi-segmented
ion trap | 17 pages, 11 figures | null | 10.1088/1367-2630/10/4/045007 | null | quant-ph | null | Miniaturized ion trap arrays with many trap segments present a promising
architecture for scalable quantum information processing. The miniaturization
of segmented linear Paul traps allows partitioning the microtrap in different
storage and processing zones. The individual position control of many ions -
each of them carrying qubit information in its long-lived electronic levels -
by the external trap control voltages is important for the implementation of
next generation large-scale quantum algorithms.
We present a novel scalable microchip multi-segmented ion trap with two
different adjacent zones, one for the storage and another dedicated for the
processing of quantum information using single ions and linear ion crystals: A
pair of radio-frequency driven electrodes and 62 independently controlled DC
electrodes allows shuttling of single ions or linear ion crystals with
numerically designed axial potentials at axial and radial trap frequencies of a
few MHz. We characterize and optimize the microtrap using sideband spectroscopy
on the narrow S1/2 <-> D5/2 qubit transition of the 40Ca+ ion, demonstrate
coherent single qubit Rabi rotations and optical cooling methods. We determine
the heating rate using sideband cooling measurements to the vibrational ground
state which is necessary for subsequent two-qubit quantum logic operations. The
applicability for scalable quantum information processing is proven.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 18:16:08 GMT"
},
{
"version": "v2",
"created": "Wed, 19 Dec 2007 23:38:16 GMT"
},
{
"version": "v3",
"created": "Sun, 3 Feb 2008 20:26:40 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schulz",
"Stephan",
""
],
[
"Poschinger",
"Ulrich",
""
],
[
"Ziesel",
"Frank",
""
],
[
"Schmidt-Kaler",
"Ferdinand",
""
]
] | [
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712.325 | Edyta Podlewska | E. Podlewska and E. Szuszkiewicz (Institute of Physics and CASA*,
University of Szczecin, Poland) | Jupiter and Super-Earth embedded in a gaseous disc | 10 pages with 8 figures, accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.12871.x | null | astro-ph | null | In this paper we investigate the evolution of a pair of interacting planets -
a Jupiter mass planet and a Super-Earth with the 5.5 Earth masses - orbiting a
Solar type star and embedded in a gaseous protoplanetary disc. We focus on the
effects of type I and II orbital migrations, caused by the planet-disc
interaction, leading to the Super-Earth capture in first order mean motion
resonances by the Jupiter. The stability of the resulting resonant system in
which the Super-Earth is on the internal orbit relatively to the Jupiter has
been studied numerically by means of full 2D hydrodynamical simulations. Our
main motivation is to determine the Super-Earth behaviour in the presence of
the gas giant in the system. It has been found that the Jupiter captures the
Super-Earth into the interior 3:2 or 4:3 mean motion resonances and the
stability of such configurations depends on the initial planet positions and
eccentricity evolution. If the initial separation of planet orbits is larger or
close to that required for the exact resonance than the final outcome is the
migration of the pair of planets with the rate similar to that of the gas giant
at least for time of our simulations. Otherwise we observe a scattering of the
Super-Earth from the disc. The evolution of planets immersed in the gaseous
disc has been compared with their behaviour in the case of the classical
three-body problem when the disc is absent.
| [
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] | 2009-11-13T00:00:00 | [
[
"Podlewska",
"E.",
"",
"Institute of Physics and CASA*,\n University of Szczecin, Poland"
],
[
"Szuszkiewicz",
"E.",
"",
"Institute of Physics and CASA*,\n University of Szczecin, Poland"
]
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712.3251 | Robert Carroll | Robert Carroll | Remarks on the Friedman equations | 13 pages, Latex, typos corrected | null | null | null | math-ph math.MP | null | We give some heuristic results for FRW situations with Ricci flow.
| [
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712.3252 | Valerio Faraoni | Valerio Faraoni and Nicolas Lanahan-Tremblay (Bishop's University) | Comments on "Solar System constraints to general f(R) gravity" | 2 latex pages, to appear in the Comments section of Phys. Rev. D. A
statement corrected, acknowledgments updated | Phys.Rev.D77:108501,2008 | 10.1103/PhysRevD.77.108501 | null | gr-qc | null | We comment on, and complete, the analysis of the weak field limit of metric
f(R) gravity in T. Chiba, T.L. Smith, and A.L. Erickcek, Phys. Rev. D 75,
124014 (2007).
| [
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{
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] | 2008-11-26T00:00:00 | [
[
"Faraoni",
"Valerio",
"",
"Bishop's University"
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[
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"Bishop's University"
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] |
712.3253 | Miron Amusia | M. Ya. Amusia (1 and 2), A. S. Baltenkov (3), L. V. Chernysheva ((1)
Hebrew University, Jerusalem, Israel, (2) Ioffe Physical-Technical Institute,
St. Petersburg, Russia, (3) Arifov Institute of Electronics, Tashkent,
Uzbekistan) | Destruction and Resurrection of Atomic Giant resonances in Endohedral
Atoms A@C60 | 25 pages, 29 figures | null | null | null | physics.atm-clus physics.atom-ph | null | It is demonstrated that in photoabsorption by endohedral atoms some atomic
Giant resonances are almost completely destroyed while the others are totally
preserved due to different action on it of the fullerenes shell. As the first
example we discuss the 4d10 Giant resonance in Xe@C60 whereas as the second
serves the Giant autoionization resonance in Eu@C60. The qualitative difference
comes from the fact that photoelectrons from the 4d Giant resonance has small
energies (tens of eV) and are strongly reflected by the C60 fullerenes shell.
As to the Eu@C60, Giant autoionization leads to fast photoelectrons (about
hundred eV) that go out almost untouched by the C60 shell. As a result of the
outgoing electrons energy difference the atomic Giant resonances will be
largely destroyed in A@C60 while the Giant autoionization resonance will be
almost completely preserved. Thus, on the way from Xe@C60 Giant resonance to
Eu@C60 Giant autoionization resonance the oscillation structure should
disappear. Similar will be the decrease of oscillations on the way from pure
Giant to pure Giant autoionization resonances for the angular anisotropy
parameters. At Giant resonance frequencies the role of polarization of the
fullerenes shell by the incoming photon beam is inessential. Quite different is
the situation for the outer electrons in Eu@C60, the photoionization of which
will be also considered.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 18:46:56 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Amusia",
"M. Ya.",
"",
"1 and 2"
],
[
"Baltenkov",
"A. S.",
""
],
[
"Chernysheva",
"L. V.",
""
]
] | [
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] |
712.3254 | Carlo Barbieri | C. Barbieri (1), E. Caurier (2), K. Langanke (1,2), G.
Mart\'inez-Pinedo (1) ((1) GSI, (2) IRES Strasbourg, (3) TU Darmstadt) | Pygmy dipole response of proton rich argon beyond the random phase
approximation | Submitted to Phys. Rev. C | null | null | null | nucl-th | null | The occurrence of a pygmy dipole resonance in proton rich Ar-32 and Ar-34 is
studied using the unitary correlator operator method interaction Vucom, based
on Argonne V18. Predictions from the random phase approximation (RPA) and the
shell model in a no-core basis are compared.
It is found that the inclusion of configuration mixing up to
two-particle--two-holes broadens the pygmy strength slightly and reduces
sensibly its strength, as compared to the RPA predictions. For Ar-32 a clear
peak associated with a pygmy resonance is found. For Ar-34, the pygmy states
are obtained close to the giant dipole resonance and mix with it.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 18:55:33 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Barbieri",
"C.",
"",
"GSI"
],
[
"Caurier",
"E.",
"",
"IRES Strasbourg"
],
[
"Langanke",
"K.",
"",
"GSI",
"IRES Strasbourg"
],
[
"Martínez-Pinedo",
"G.",
"",
"GSI"
]
] | [
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] |
712.3255 | Georgios Mountrichas | Georgios Mountrichas, Tom Shanks | Clustering of 2PIGG galaxy groups with 2dFGRS galaxies | 20 pages, 32 figures, 9 tables | null | 10.1111/j.1365-2966.2009.15162.x | null | astro-ph | null | Prompted by indications from QSO lensing that there may be more mass
associated with galaxy groups than expected, we have made new dynamical infall
estimates of the masses associated with 2PIGG groups and clusters. We have
analysed the redshift distortions in the cluster-galaxy cross-correlation
function as a function of cluster membership, cross-correlating z<0.12 2PIGG
clusters and groups with the full 2dF galaxy catalogue. We have made estimates
of the dynamical infall parameter beta and new estimates of the group velocity
dispersions. We first find that the amplitude of the full 3-D redshift space
cross-correlation function, xi_{cg}, rises monotonically with group membership.
We use a simple linear-theory infall model to fit xi(sigma, pi) in the range
5<s<40h^{-1}Mpc. We find that the beta versus membership relation for the data
shows a minimum at intermediate group membership n~20 or L~2x10^11h^-2Lsun,
implying that the bias and hence M/L ratios rise by a significant factor (~5x)
both for small groups and rich clusters. However, the mocks show a systematic
shift between the location of the beta minimum and the M/L minimum at
L~10^10h^-2Lsun given by direct calculation using the known DM distribution.
Our overall conclusion is that bias estimates from dynamical infall appear to
support the minimum in star-formation efficiency at intermediate halo masses.
Nevertheless, there may still be significant systematic problems arising from
measuring beta~1/b using large-scale infall rather than M/L using small-scale
velocity dispersions.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:32:40 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Mountrichas",
"Georgios",
""
],
[
"Shanks",
"Tom",
""
]
] | [
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] |
712.3256 | Gregory F. Lawler | Gregory F. Lawler | Schramm-Loewner Evolution | Lecture notes from course given at Park City/IAS Institute, Park
City, Utah, 2007 | null | null | null | math.PR | null | This is the first expository set of notes on SLE I have written since
publishing a book two years ago [45]. That book covers material from a
year-long class, so I cannot cover everything there. However, these notes are
not just a subset of those notes, because there is a slight change of
perspective. The main differences are:
o I have defined SLE as a finite measure on paths that is not necessarily a
probability measure. This seems more natural from the perspective of limits of
lattice systems and seems to be more useful when extending SLE to non-simply
connected domains. (However, I do not discuss non-simply connected domains in
these notes.)
o I have made more use of the Girsanov theorem in studying corresponding
martingales and local martingales.
As in [45], I will focus these notes on the continuous process SLE and will
not prove any results about convergence of discrete processes to SLE. However,
my first lecture will be about discrete processes -- it is very hard to
appreciate SLE if one does not understand what it is trying to model.
| [
{
"version": "v1",
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] | 2007-12-20T00:00:00 | [
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712.3257 | Manfred Cuntz | M. Cuntz, L. Gurdemir, E. F. Guinan, R. L. Kurucz | Astrobiological Effects of F, G, K and M Main-Sequence Stars | 3 pages, 3 figures; submitted to: Exoplanets: Detection, Formation
and Dynamics, IAU Symposium 249, eds. Y.S. Sun and S. Ferraz-Mello (San
Francisco: Astr. Soc. Pac.) | null | 10.1017/S174392130801661X | null | astro-ph | null | We focus on the astrobiological effects of photospheric radiation produced by
main-sequence stars of spectral types F, G, K, and M. The photospheric
radiation is represented by using realistic spectra, taking into account
millions or hundred of millions of lines for atoms and molecules. DNA is taken
as a proxy for carbon-based macromolecules, assumed to be the chemical
centerpiece of extraterrestrial life forms. Emphasis is placed on the
investigation of the radiative environment in conservative as well as
generalized habitable zones.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:54:21 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 21:04:03 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cuntz",
"M.",
""
],
[
"Gurdemir",
"L.",
""
],
[
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"E. F.",
""
],
[
"Kurucz",
"R. L.",
""
]
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712.3258 | Nicolo' Antonietti | N. Antonietti, M. Mondin, G. Catastini, G. Brida, and M. Genovese | Systematic Numerical Study of the Propagation of Monochromatic Radiation
through a Stationary Atmosphere in a Model of Plane Plane-Parallel Layers | null | Laser Physics, 2007, Vol. 17, No. 12, pp. 1389-1397 | 10.1134/S1054660X07120092 | null | physics.optics quant-ph | null | In this paper, the authors compare the security bounds for different quantum
communication protocols with the numerically evaluated losses in the
transmission channel, due to the interaction between the atmosphere and the
photon, which is the information carrier. The analysis is carried out using a
free-source library, which can solve the radiative transfer equation for a
parallel-plane atmosphere.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:12:35 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Dec 2007 20:17:02 GMT"
}
] | 2008-01-02T00:00:00 | [
[
"Antonietti",
"N.",
""
],
[
"Mondin",
"M.",
""
],
[
"Catastini",
"G.",
""
],
[
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"G.",
""
],
[
"Genovese",
"M.",
""
]
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] |
712.3259 | Johan Nilsson | Johan Nilsson, A. H. Castro Neto, F. Guinea, N. M. R. Peres | Electronic properties of bilayer and multilayer graphene | 36 pages, 42 figures, references added | Phys. Rev. B 78, 045405 (2008) | 10.1103/PhysRevB.78.045405 | null | cond-mat.mes-hall | null | We study the effects of site dilution disorder on the electronic properties
in graphene multilayers, in particular the bilayer and the infinite stack. The
simplicity of the model allows for an easy implementation of the coherent
potential approximation and some analytical results. Within the model we
compute the self-energies, the density of states and the spectral functions.
Moreover, we obtain the frequency and temperature dependence of the
conductivity as well as the DC conductivity. The c-axis response is
unconventional in the sense that impurities increase the response for low
enough doping. We also study the problem of impurities in the biased graphene
bilayer.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:01:03 GMT"
},
{
"version": "v2",
"created": "Thu, 24 Jan 2008 14:46:21 GMT"
}
] | 2008-07-03T00:00:00 | [
[
"Nilsson",
"Johan",
""
],
[
"Neto",
"A. H. Castro",
""
],
[
"Guinea",
"F.",
""
],
[
"Peres",
"N. M. R.",
""
]
] | [
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] |
712.326 | Manfred Cuntz | M. Cuntz, L. Gurdemir, E.F. Guinan, R. L. Kurucz | Astrobiology in the Environments of Main-Sequence Stars: Effects of
Photospheric Radiation | 4 pages, 4 figures; submitted to: Bioastronomy 2007: Molecules,
Microbes and Extraterrestrial Life, eds. K. Meech, M. Mumma, J. Siefert and
D. Werthimer, A.S.P. Conf. Ser | null | null | null | astro-ph | null | We explore if carbon-based macromolecules (such as DNA) in the environments
of stars other than the Sun are able to survive the effects of photospheric
stellar radiation, such as UV-C. Therefore, we focus on main-sequence stars of
spectral types F, G, K, and M. Emphasis is placed on investigating the
radiative environment in the stellar habitable zones. Stellar habitable zones
are relevant to astrobiology because they constitute circumstellar regions in
which a planet of suitable size can maintain surface temperatures for water to
exist in fluid form, thus increasing the likelihood of Earth-type life.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:25:24 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Cuntz",
"M.",
""
],
[
"Gurdemir",
"L.",
""
],
[
"Guinan",
"E. F.",
""
],
[
"Kurucz",
"R. L.",
""
]
] | [
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] |
712.3261 | Marcin Bilski | Marcin Bilski | Algebraic approximation of analytic sets and mappings | 23 pages | J. Math. Pures Appl. 90 (2008) 312-327 | null | null | math.CV | null | Let {X_n} be a sequence of analytic sets converging to some analytic set X in
the sense of holomorphic chains. We introduce a condition which implies that
every irreducible component of X is the limit of a sequence of irreducible
components of the sets from {X_n}. Next we apply the condition to approximate a
holomorphic solution y=f(x) of a system Q(x,y)=0 of Nash equations by Nash
solutions. Presented methods allow to construct an algorithm of approximation
of the holomorphic solutions.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:25:40 GMT"
}
] | 2008-10-23T00:00:00 | [
[
"Bilski",
"Marcin",
""
]
] | [
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] |
712.3262 | Wei Wu | Wei Wu, A. Kerridge, A. H. Harker and A. J. Fisher | Structure-dependent exchange in the organic magnets Cu(II)Pc and
Mn(II)Pc | 13 pages,10 figures. To appear in Physical Review B | null | 10.1103/PhysRevB.77.184403 | QIP07_WW3_CuPcMnPc | cond-mat.mtrl-sci | null | We study exchange couplings in the organic magnets copper(II) phthalocyanine
(Cu(II)Pc) and manganese(II) phthalocyanine (Mn(II)Pc) by a combination of
Green's function perturbation theory and \textsl{ab initio} density-functional
theory (DFT). Based on the indirect exchange model our perturbation-theory
calculation of Cu(II)Pc qualitatively agrees with the experimental
observations. DFT calculations performed on Cu(II)Pc dimer show a very good
quantitative agreement with exchange couplings that we extract by using a
global fitting for the magnetization measurements to a spin-1/2 Bonner-Fisher
model. These two methods give us remarkably consistent trends for the exchange
couplings in Cu(II)Pc when changing the stacking angles. The situation is more
complex for Mn(II)Pc owing to the competition between super-exchange and
indirect exchange.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:52:34 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Mar 2008 19:48:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wu",
"Wei",
""
],
[
"Kerridge",
"A.",
""
],
[
"Harker",
"A. H.",
""
],
[
"Fisher",
"A. J.",
""
]
] | [
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] |
712.3263 | Gregory F. Lawler | Gregory F. Lawler | Dimension and natural parametrization for SLE curves | null | null | null | null | math.PR math-ph math.MP | null | Some possible definitions for the natural parametrization of SLE
(Schramm-Loewner evolution) paths are proposed in terms of various limits. One
of the definitions is used to give a new proof of the Hausdorff dimension of
SLE paths.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:32:04 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Lawler",
"Gregory F.",
""
]
] | [
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] |
712.3264 | Elizabeth Untiedt | Elizabeth Untiedt and Weldon Lodwick | Using Gradual Numbers to Analyze Non-Monotonic Functions of Fuzzy
Intervals | null | null | null | null | math.OC | null | Gradual numbers have been introduced recently as a means of extending
standard interval computation methods to fuzzy intervals. The literature treats
monotonic functions of fuzzy intervals. In this paper, we combine the concepts
of gradual numbers and optimization, which allows for the evaluation of any
differentiable function on fuzzy intervals, with no monotonicity requirement.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:32:45 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Untiedt",
"Elizabeth",
""
],
[
"Lodwick",
"Weldon",
""
]
] | [
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] |
712.3265 | Pietro Slavich | G. Degrassi, P. Gambino and P. Slavich | SusyBSG: a fortran code for BR[B -> Xs gamma] in the MSSM with Minimal
Flavor Violation | 27 pages, 2 figures; v2 to appear in Comput.Phys.Commun. - refers to
version 1.1 of the code; v3: note added on title page | Comput.Phys.Commun.179:759-771,2008 | 10.1016/j.cpc.2008.06.012 | RM3-TH/07-19, DFTT-28/2007, LAPTH-1225/07, CERN-PH-TH/2007-265 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present the fortran code SusyBSG version 1.1, which computes the branching
ratio for the decay B -> Xs gamma in the MSSM with Minimal Flavor Violation.
The computation takes into account all the available NLO contributions,
including the complete supersymmetric QCD corrections to the Wilson
coefficients of the magnetic and chromomagnetic operators.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:36:23 GMT"
},
{
"version": "v2",
"created": "Mon, 23 Jun 2008 13:59:49 GMT"
},
{
"version": "v3",
"created": "Mon, 14 Feb 2011 12:06:03 GMT"
}
] | 2011-02-15T00:00:00 | [
[
"Degrassi",
"G.",
""
],
[
"Gambino",
"P.",
""
],
[
"Slavich",
"P.",
""
]
] | [
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] |
712.3266 | Manfred Cuntz | J. Eberle, M. Cuntz, Z. E. Musielak | Orbital Stability of Earth-Type Planets in Binary Systems | 4 pages, 1 figure; submitted to: Bioastronomy 2007: Molecules,
Microbes and Extraterrestrial Life, eds. K. Meech, M. Mumma, J. Siefert and
D. Werthimer, A.S.P. Conf. Ser | null | null | null | astro-ph | null | About half of all known stellar systems with Sun-like stars consist of two or
more stars, significantly affecting the orbital stability of any planet in
these systems. Here we study the onset of instability for an Earth-type planet
that is part of a binary system. Our investigation makes use of previous
analytical work allowing to describe the permissible region of planetary
motion. This allows us to establish a criterion for the orbital stability of
planets that may be useful in the context of future observational and
theoretical studies.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:38:49 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Eberle",
"J.",
""
],
[
"Cuntz",
"M.",
""
],
[
"Musielak",
"Z. E.",
""
]
] | [
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] |
712.3267 | Alberto Girlando | A. Girlando, M. Masino, A. Painelli, N. Drichko, M. Dressel, A.
Brillante, R. G. Della Valle, and E. Venuti | Direct evidence of overdamped Peierls-coupled modes in TTF-CA
temperature-induced phase transition | 11 pages, 13 figures | Phys. Rev. B 78, 045103 (2008) | 10.1103/PhysRevB.78.045103 | null | cond-mat.other | null | In this paper we elucidate the optical response resulting from the interplay
of charge distribution (ionicity) and Peierls instability (dimerization) in the
neutral-ionic, ferroelectric phase transition of tetrathiafulvalene-chloranil
(TTF-CA), a mixed-stack quasi-one-dimensional charge-transfer crystal. We
present far-infrared reflectivity measurements down to 5 cm-1 as a function of
temperature above the phase transition (300 - 82 K). The coupling between
electrons and lattice phonons in the pre-transitional regime is analyzed on the
basis of phonon eigenvectors and polarizability calculations of the
one-dimensional Peierls-Hubbard model. We find a multi-phonon Peierls coupling,
but on approaching the transition the spectral weight and the coupling shift
progressively towards the phonons at lower frequencies, resulting in a
soft-mode behavior only for the lowest frequency phonon near the transition
temperature. Moreover, in the proximity of the phase transition, the
lowest-frequency phonon becomes overdamped, due to anharmonicity induced by its
coupling to electrons. The implications of these findings for the neutral-ionic
transition mechanism is shortly discussed.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 19:46:04 GMT"
}
] | 2021-11-23T00:00:00 | [
[
"Girlando",
"A.",
""
],
[
"Masino",
"M.",
""
],
[
"Painelli",
"A.",
""
],
[
"Drichko",
"N.",
""
],
[
"Dressel",
"M.",
""
],
[
"Brillante",
"A.",
""
],
[
"Della Valle",
"R. G.",
""
],
[
"Venuti",
"E.",
""
]
] | [
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] |
712.3268 | Adan Cabello | Adan Cabello, David Rodriguez, Ignacio Villanueva | Necessary and sufficient detection efficiency for the Mermin
inequalities | REVTeX4, 5 pages, 1 figure | Phys. Rev. Lett. 101 (2008) 120402 | 10.1103/PhysRevLett.101.120402 | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove that the threshold detection efficiency for a loophole-free Bell
experiment using an $n$-qubit Greenberger-Horne-Zeilinger state and the
correlations appearing in the $n$-partite Mermin inequality is $n/(2n-2)$. If
the detection efficiency is equal to or lower than this value, there are local
hidden variable models that can simulate all the quantum predictions. If the
detection efficiency is above this value, there is no local hidden variable
model that can simulate all the quantum predictions.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:23:46 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Dec 2007 19:42:28 GMT"
},
{
"version": "v3",
"created": "Wed, 23 Jan 2008 19:33:19 GMT"
},
{
"version": "v4",
"created": "Wed, 9 Apr 2008 23:03:55 GMT"
},
{
"version": "v5",
"created": "Tue, 16 Sep 2008 14:30:32 GMT"
}
] | 2009-07-28T00:00:00 | [
[
"Cabello",
"Adan",
""
],
[
"Rodriguez",
"David",
""
],
[
"Villanueva",
"Ignacio",
""
]
] | [
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] |
712.3269 | Houri Ziaeepour | Houri Ziaeepour, Stephen T. Holland, Patricia T. Boyd, Kim L. Page,
Samantha Oates, Craig B. Markwardt, Peter Meszaros, Neil Gehrels, Francis E.
Marshall, Jay Cummings, Mike Goad | GRB 060607A: A GRB with Bright Asynchronous Early $X$-ray and Optical
Emissions | 17 pages; 9 figures; Accepted for publication in MNRAS | Mon.Not.Roy.Astron.Soc.385:453,2008 | 10.1111/j.1365-2966.2008.12859.x | null | astro-ph | null | The early optical emission of the moderately high redshift ($z=3.08$) GRB
060607A shows a remarkable broad and strong peak with a rapid rise and a
relatively slow power-law decay. It is not coincident with the strong
early-time flares seen in the X-ray and gamma-ray energy bands. There is weak
evidence for variability superposed on this dominant component in several
optical bands that can be related to flares in high energy bands. While for a
small number of GRBs, well-sampled optical flares have been observed
simultaneously with X-ray and gamma ray pulses, GRB 060607A is one of the few
cases where the early optical emission shows no significant evidence for
correlation with the prompt emission. In this work we first report in detail
the broad band observations of this burst by Swift. Then by applying a simple
model for the dynamics and the synchrotron radiation of a relativistic shock,
we show that the dominant component of the early emissions in optical
wavelengths has the same origin as the tail emission produced after the main
gamma ray activity. The most plausible explanation for the peak in the optical
light curve seems to be the cooling of the prompt after the main collisions,
shifting the characteristic synchrotron frequency to the optical bands. It
seems that the cooling process requires a steepening of the electron energy
distribution and/or a break in this distribution at high energies. The sharp
break in the X-ray light curve at few thousands of seconds after the trigger,
is not observed in the IR/optical/UV bands, and therefore can not be a jet
break. Either the X-ray break is due to a change in the spectrum of the
accelerated electrons or the lack of an optical break is due to the presence of
a related delayed response component (Abbreviated).
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:24:27 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Ziaeepour",
"Houri",
""
],
[
"Holland",
"Stephen T.",
""
],
[
"Boyd",
"Patricia T.",
""
],
[
"Page",
"Kim L.",
""
],
[
"Oates",
"Samantha",
""
],
[
"Markwardt",
"Craig B.",
""
],
[
"Meszaros",
"Peter",
""
],
[
"Gehrels",
"Neil",
""
],
[
"Marshall",
"Francis E.",
""
],
[
"Cummings",
"Jay",
""
],
[
"Goad",
"Mike",
""
]
] | [
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712.327 | Manfred Cuntz | S. H. Saar, M. Cuntz, V. L. Kashyap, J. C. Hall | First Observation of Planet-Induced X-ray Emission: The System HD 179949 | 3 pages, 1 figure; Exoplanets: Detection, Formation and Dynamics, IAU
Symposium 249, eds. Y.-S. Sun, S. Ferraz-Mello, and J.-L. Zhou (Cambridge:
Cambridge University Press) | null | 10.1017/S1743921308016414 | null | astro-ph | null | We present the first observation of planet-induced stellar X-ray activity,
identified for the HD 179949 system, using Chandra / ACIS-S. The HD 179949
system consists of a close-in giant planet orbiting an F9V star. Previous
ground-based observations already showed enhancements in Ca II K in phase with
the planetary orbit. We find an ~30% increase in the X-ray flux over quiescent
levels coincident with the phase of the Ca II enhancements. There is also a
trend for the emission to be hotter at increased fluxes, confirmed by modeling,
showing the enhancement at ~1 keV compared to ~0.4 keV for the background star.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:45:31 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 21:30:32 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Saar",
"S. H.",
""
],
[
"Cuntz",
"M.",
""
],
[
"Kashyap",
"V. L.",
""
],
[
"Hall",
"J. C.",
""
]
] | [
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712.3271 | H. J. Carmichael | Changsuk Noh and H. J. Carmichael | Disentanglement of Source and Target and the Laser Quantum State | 4 pages, 1 figure | Phys. Rev. Lett. 100, 120405(2008) | 10.1103/PhysRevLett.100.120405 | null | quant-ph | null | Disentanglement of a laser source from its target qubit is proposed as a
criterion establishing the laser quantum state as a coherent state. It is shown
that the source-target density operator has a unique factorization in coherent
states when the environmental record monitoring laser pump quanta is ignored.
The source-target state conditioned upon the complete environmental record is
entangled, though, as a state of known total quanta number (source plus
target).
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:33:54 GMT"
}
] | 2008-09-24T00:00:00 | [
[
"Noh",
"Changsuk",
""
],
[
"Carmichael",
"H. J.",
""
]
] | [
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712.3272 | Ilarion Melnikov | Jock McOrist and Ilarion V. Melnikov | Half-Twisted Correlators from the Coulomb Branch | 21 pages, LaTex; typos corrected; some discussion added | JHEP 0804:071,2008 | 10.1088/1126-6708/2008/04/071 | EFI-07-40 | hep-th | null | We compute correlators of chiral operators in half-twisted (0,2)
supersymmetric gauged linear sigma models. Our results give simple algebraic
formulas for a (0,2) generalization of genus zero Gromov-Witten invariants of
compact toric varieties. We derive compact expressions for deformed quantum
cohomology relations and apply our general method to several examples.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:34:34 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Dec 2007 20:08:25 GMT"
},
{
"version": "v3",
"created": "Tue, 12 Feb 2008 21:36:28 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"McOrist",
"Jock",
""
],
[
"Melnikov",
"Ilarion V.",
""
]
] | [
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] |
712.3273 | Shabnaz Pashapour | CDF Collaboration: T. Aaltonen, et al | First Measurement of the Fraction of Top Quark Pair Production Through
Gluon-Gluon Fusion | 6 pages, 2 figures, Submitted to Phys.Rev.Lett, added 95% CL upper
limit | Phys.Rev.D78:111101,2008 | 10.1103/PhysRevD.78.111101 | FERMILAB-PUB-07-665-E | hep-ex | null | We present the first measurement of the fraction of top quark pair production
through gluon-gluon fusion. We use 0.96/fb of s**(1/2)=1.96 TeV p-pbar
collision data recorded with the CDF II detector at Fermilab. We identify the
candidate t-tbar events with a high-energy charged lepton, a neutrino
candidate, and four or more jets. Using charged particles with low transverse
momentum in t-tbar events, we find the fraction of top quark pair production
through gluon-gluon fusion to be 0.07+/-0.14(stat)+/-0.07(syst), corresponding
to a 95% confidence level upper limit of 0.33, in agreement with the standard
model NLO prediction of 0.15+/-0.05.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:36:32 GMT"
},
{
"version": "v2",
"created": "Tue, 8 Apr 2008 13:34:48 GMT"
}
] | 2010-05-12T00:00:00 | [
[
"CDF Collaboration",
"",
""
],
[
"Aaltonen",
"T.",
""
]
] | [
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712.3274 | Dirk Kussin | Dirk Kussin | Parameter curves for the regular representations of tame bimodules | 13 pages, to appear in J. Algebra. Typos corrected | null | 10.1016/j.jalgebra.2008.05.022 | null | math.RT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present results and examples which show that the consideration of a
certain tubular mutation is advantageous in the study of noncommutative curves
which parametrize the simple regular representations of a tame bimodule. We
classify all tame bimodules where such a curve is actually commutative, or in
different words, where the unique generic module has a commutative endomorphism
ring. This extends results from [14] to arbitrary characteristic; in
characteristic two additionally inseparable cases occur. Further results are
concerned with autoequivalences fixing all objects but not isomorphic to the
identity functor.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:41:35 GMT"
},
{
"version": "v2",
"created": "Tue, 19 Feb 2008 16:14:25 GMT"
},
{
"version": "v3",
"created": "Mon, 16 Jun 2008 20:03:48 GMT"
}
] | 2008-06-16T00:00:00 | [
[
"Kussin",
"Dirk",
""
]
] | [
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] |
712.3275 | Sean Sather-Wagstaff | Anders J. Frankild, Sean Sather-Wagstaff and Amelia Taylor | Relations between semidualizing complexes | final version, to appear in J. Commutative Algebra, 27 pages, uses
XY-pic | null | null | null | math.AC | null | We study the following question: Given two semidualizing complexes B and C
over a commutative noetherian ring R, does the vanishing of Ext^n_R(B,C) for
n>>0 imply that B is C-reflexive? This question is a natural generalization of
one studied by Avramov, Buchweitz, and Sega. We begin by providing conditions
equivalent to B being C-reflexive, each of which is slightly stronger than the
condition Ext^n_R(B,C)=0 for all n>>0. We introduce and investigate an
equivalence relation \approx on the set of isomorphism classes of semidualizing
complexes. This relation is defined in terms of a natural action of the derived
Picard group and is well-suited for the study of semidualizing complexes over
nonlocal rings. We identify numerous alternate characterizations of this
relation, each of which includes the condition Ext^n_R(B,C)=0 for all n>>0.
Finally, we answer our original question in some special cases.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:44:33 GMT"
},
{
"version": "v2",
"created": "Fri, 7 Mar 2008 19:02:30 GMT"
}
] | 2008-03-07T00:00:00 | [
[
"Frankild",
"Anders J.",
""
],
[
"Sather-Wagstaff",
"Sean",
""
],
[
"Taylor",
"Amelia",
""
]
] | [
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] |
712.3276 | Andrea Wulzer Dr | Alex Pomarol, Andrea Wulzer | Stable skyrmions from extra dimensions | 20 pages, 3 figures | JHEP 0803:051-051,2008 | 10.1088/1126-6708/2008/03/051 | UAB-FT-636 | hep-th hep-ph | null | We show that skyrmions arising from compact five dimensional models have
stable sizes. We numerically obtain the skyrmion configurations and calculate
their size and energy. Although their size strongly depends on the magnitude of
localized kinetic-terms, their energy is quite model-independent ranging
between 50-65 times F_pi^2/m_rho, where F_pi is the Goldstone decay constant
and m_rho the lowest Kaluza-Klein mass. These skyrmion configurations
interpolate between small 4D YM instantons and 4D skyrmions made of Goldstones
and a massive vector boson. Contrary to the original 4D skyrmion and previous
5D extensions, these configurations have sizes larger than the inverse of the
cut-off scale and therefore they are trustable within our effective 5D
approach. Such solitonic particles can have interesting phenomenological
consequences as they carry a conserved topological charge analogous to baryon
number.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:56:32 GMT"
}
] | 2009-12-15T00:00:00 | [
[
"Pomarol",
"Alex",
""
],
[
"Wulzer",
"Andrea",
""
]
] | [
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] |
712.3277 | Mustafa Cenk Gursoy | Mustafa Cenk Gursoy | On the Capacity and Energy Efficiency of Training-Based Transmissions
over Fading Channels | null | null | null | null | cs.IT math.IT | null | In this paper, the capacity and energy efficiency of training-based
communication schemes employed for transmission over a-priori unknown Rayleigh
block fading channels are studied. In these schemes, periodically transmitted
training symbols are used at the receiver to obtain the minimum
mean-square-error (MMSE) estimate of the channel fading coefficients.
Initially, the case in which the product of the estimate error and transmitted
signal is assumed to be Gaussian noise is considered. In this case, it is shown
that bit energy requirements grow without bound as the signal-to-noise ratio
(SNR) goes to zero, and the minimum bit energy is achieved at a nonzero SNR
value below which one should not operate. The effect of the block length on
both the minimum bit energy and the SNR value at which the minimum is achieved
is investigated. Flash training and transmission schemes are analyzed and shown
to improve the energy efficiency in the low-SNR regime.
In the second part of the paper, the capacity and energy efficiency of
training-based schemes are investigated when the channel input is subject to
peak power constraints. The capacity-achieving input structure is characterized
and the magnitude distribution of the optimal input is shown to be discrete
with a finite number of mass points. The capacity, bit energy requirements, and
optimal resource allocation strategies are obtained through numerical analysis.
The bit energy is again shown to grow without bound as SNR decreases to zero
due to the presence of peakedness constraints. The improvements in energy
efficiency when on-off keying with fixed peak power and vanishing duty cycle is
employed are studied. Comparisons of the performances of training-based and
noncoherent transmission schemes are provided.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:55:29 GMT"
}
] | 2007-12-20T00:00:00 | [
[
"Gursoy",
"Mustafa Cenk",
""
]
] | [
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-0.10941457,
-0.0195401143,
-0.1328677386,
-0.1685004532,
0.0820860937,
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-0.0257934537,
0.090792954,
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0.0465037078
] |
712.3278 | Sergey Storchak | S. N. Storchak | On geometrical representation of the Jacobian in a path integral
reduction problem | 8 pages | null | 10.1016/j.physleta.2008.09.017 | null | math-ph math.MP | null | The geometrical representation of the Jacobian in the path integral reduction
problem which describes a motion of the scalar particle on a smooth compact
Riemannian manifold with the given free isometric action of the compact
semisimple Lie group is obtained. By using the formula for the scalar curvature
of the manifold with the Kaluza--Klein metric, we present the Jacobian as
difference of the scalar curvature of the total space of the principal fibre
bundle and the terms that are the scalar curvature of the orbit space, the
scalar curvature of the orbit, the second fundamental form of the orbit and the
square of the principle fibre bundle curvature.
| [
{
"version": "v1",
"created": "Wed, 19 Dec 2007 20:57:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Storchak",
"S. N.",
""
]
] | [
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